- published: 25 Nov 2015
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An active galactic nucleus (AGN) is a compact region at the centre of a galaxy that has a much higher than normal luminosity over at least some portion – and possibly all – of the electromagnetic spectrum. Such excess emission has been observed in the radio, microwaves, infrared, optical, ultra-violet, X-ray and gamma ray wavebands. A galaxy hosting an AGN is called an active galaxy. The radiation from an AGN is believed to be a result of accretion of mass by a supermassive black hole at the centre of its host galaxy. AGN are the most luminous persistent sources of electromagnetic radiation in the universe, and as such can be used as a means of discovering distant objects; their evolution as a function of cosmic time also puts constraints on models of the cosmos.
For a long time it has been argued that an AGN must be powered by accretion of mass onto massive black holes (106 to 1010 times the Solar mass). AGN are both compact and persistently extremely luminous. Accretion can potentially give very efficient conversion of potential and kinetic energy to radiation, and a massive black hole has a high Eddington luminosity, and as a result, it can provide the observed high persistent luminosity. Supermassive black holes are now believed to exist in the centres of most if not all massive galaxies since the mass of the black hole correlates well with the velocity dispersion of the galactic bulge (the M-sigma relation) or with bulge luminosity. Thus AGN-like characteristics are expected whenever a supply of material for accretion comes within the sphere of influence of the central black hole.
Active may refer to:
A hole is an opening.
Hole or holes may also refer to:
Crash Course (also known as Driving Academy) is a 1988 made for television teen film directed by Oz Scott.
Crash Course centers on a group of high schoolers in a driver’s education class; many for the second or third time. The recently divorced teacher, super-passive Larry Pearl, is on thin ice with the football fanatic principal, Principal Paulson, who is being pressured by the district superintendent to raise driver’s education completion rates or lose his coveted football program. With this in mind, Principal Paulson and his assistant, with a secret desire for his job, Abner Frasier, hire an outside driver’s education instructor with a very tough reputation, Edna Savage, aka E.W. Savage, who quickly takes control of the class.
The plot focuses mostly on the students and their interactions with their teachers and each other. In the beginning, Rico is the loner with just a few friends, Chadley is the bookish nerd with few friends who longs to be cool and also longs to be a part of Vanessa’s life who is the young, friendly and attractive girl who had to fake her mother’s signature on her driver’s education permission slip. Kichi is the hip-hop Asian kid who often raps what he has to say and constantly flirts with Maria, the rich foreign girl who thinks that the right-of-way on the roadways always goes to (insert awesomely fake foreign Latino accent) “my father’s limo”. Finally you have stereotypical football meathead J.J., who needs to pass his English exam to keep his eligibility and constantly asks out and gets rejected by Alice, the tomboy whose father owns “Santini & Son” Concrete Company. Alice is portrayed as being the “son” her father wanted.
Creative Commons (CC) is a non-profit organization devoted to expanding the range of creative works available for others to build upon legally and to share. The organization has released several copyright-licenses known as Creative Commons licenses free of charge to the public. These licenses allow creators to communicate which rights they reserve, and which rights they waive for the benefit of recipients or other creators. An easy-to-understand one-page explanation of rights, with associated visual symbols, explains the specifics of each Creative Commons license. Creative Commons licenses do not replace copyright, but are based upon it. They replace individual negotiations for specific rights between copyright owner (licensor) and licensee, which are necessary under an "all rights reserved" copyright management, with a "some rights reserved" management employing standardized licenses for re-use cases where no commercial compensation is sought by the copyright owner. The result is an agile, low-overhead and low-cost copyright-management regime, profiting both copyright owners and licensees. Wikipedia uses one of these licenses.
Hello and welcome to What Da Math! In this video, we will talk about new various AGN objects such as Quasars, Blazars and Radio Galaxies and how to make them in Universe Sandbox 2. Enjoy and please subscribe. Buy the game here: http://store.steampowered.com/app/230290 Twitter: https://twitter.com/WhatDaMath Facebook: https://www.facebook.com/whatdamath Twitch: http://www.twitch.tv/whatdamath Patreon page: https://www.patreon.com/user?u=2318196&ty;=h Other videos here: https://www.youtube.com/playlist?list=PL9hNFus3sjE7jgrGJYkZeTpR7lnyVAk-x
These lectures give an in-depth observational overview of Active Galactic Nuclei (AGNs). Topics include the following: Introduction; AGN Basics; Finding AGNs; Terminology; The Black Hole Region; The Broad Line Region; Outflowing Winds; The Narrow Line Region; The Torus; Jets; and AGN Demography, Physics, and Ecology from X-ray Surveys. The total lecturing time is about 10.5 hours, and the lecturer is Prof. William N. Brandt (Penn State). There are two YouTube parts to these lectures. These lectures were presented from 2014 June 23-27 at the USTC Summer School on "Formation and Co-Evolution of Galaxies and Supermassive Black Holes" in Hefei, China. The lead organizer of the summer school was Prof. Yongquan Xue (USTC). See http://smbh2014.csp.escience.cn/dct/page/1 for details about the su...
A long time ago in a galaxy far, far away, something was feeding. That something was a supermassive black hole. When these things snack, they have the potential to outshine their entire host galaxy and it is this light that we can observe today. Termed Active Galactic Nuclei, they provide astronomers with evidence of extreme physical processes which are not yet fully understood. This will be a gentle introduction to the subject of AGN and how they have contributed to our understanding of the Universe. The lecture by Alastair Bruce was sponsored by the Institute of Physics in Scotland. It was recorded at Robert Gordon's College, Aberdeen, on Monday 5th October 2015.
Active galaxies pour out lots of energy, due to their central supermassive black holes gobbling down matter. Galaxies tend not to be loners, but instead exist in smaller groups and larger clusters. Our Milky Way is part of the Local Group, and will one day collide with the Andromeda galaxy. Clusters of galaxies also clump together to form superclusters, the largest structures in the Universe. In total, there are hundreds of billions of galaxies in the Universe. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Black Holes at the Center of Galaxies 2:26 Galaxies Are a Part of Small/Large Clusters 9:47 The Milky Way is Part of the Local Group 6:45 Galaxy Clusters Clump Together to Create Superclusters 11:03 Hundreds of Billion...
A team of astronomers using the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 (WFC3) have conducted a large survey to investigate the relationship between galaxies that have undergone mergers and the activity of the supermassive black holes at their cores. The team studied a large selection of galaxies with extremely luminous centres — known as active galactic nuclei (AGNs) — thought to be the result of large quantities of heated matter circling around and being consumed by a supermassive black hole. Whilst most galaxies are thought to host a supermassive black hole, only a small percentage of them are this luminous and fewer still go one step further and form what are known as relativistic jets. The two high-speed jets of plasma move almost with the speed of light and stream out i...
Most galaxies have at their cores a supermassive black hole hundreds of millions of times the mass of our Sun. They emit powerful ultraviolet radiation from the supermassive black hole at the core of the host galaxy. The most active of these galaxy cores are called quasars, where infalling material is heated to a point where a brilliant searchlight shines into deep space. The beam is produced by a disk of glowing, superheated gas encircling the black hole. Please join +Tony Darnell Dr.+Carol Christian and +Scott Lewis as they discuss some fascinating new observations of quasars made by the Hubble Space Telescope Read more here: http://hubblesite.org/newscenter/archive/releases/2015/13/ http://hubble25th.org #Hubble25 featured in Spaceport magazine: http://issuu.com/spaceportmagazine...
This simulation follows the collision of two spiral galaxies that harbor giant black holes. The collision merges the black holes and stirs up gas in both galaxies. The merged black hole gorges on the feast and lights up, forming an active galactic nucleus called a quasar and creating a "wind"" that blows away much of the galaxy's gas. "
Totally unscripted, unrehearsed, unprepared takes on the latest astronomy news stories from real scientists! Follow http://www.twitter.com/PaulMattSutter for more! Hosted by Paul Sutter (https://twitter.com/PaulMattSutter), Wayne Schlingman (https://twitter.com/stewardwildcat), Grace Calhoun (http://www.twitter.com/galacticgrace), and Anna Nierenberg (http://u.osu.edu/nierenberg.1/). Editing by Doug Dangler, OSU eLearning Program Manager. Useful links: Paul: http://www.pmsutter.com OSU: https://www.osu.edu Dept. of Physics: https://physics.osu.edu CCAPP: http://ccapp.osu.edu Dept. of Astronomy: https://astronomy.osu.edu Planetarium: https://planetarium.osu.edu College of Arts & Sciences: https://artsandsciences.osu.edu
This animation illustrates the anatomy of an active galactic nucleus powered by a supermassive black hole. The animation also shows how the viewing angle affects the appearance of the nucleus.
An "active galactic nucleus" is a compact region at the centre of a galaxy that has a much higher than normal luminosity over at least some portion – and possibly all – of the electromagnetic spectrum. Such excess emission has been observed in the radio, microwaves, infrared, optical, ultra-violet, X-ray and gamma ray wavebands. A galaxy hosting an AGN is called an "active galaxy", which is thought to be one of the candidates of high and ultra-high energy astroparticles " ". The radiation from AGN is believed to be a result of accretion of mass by a supermassive black hole at the centre of its host galaxy. AGN are the most luminous persistent sources of electromagnetic radiation in the universe, and as such can be used as a means of discovering distant objects; their evolution as a funct...
Hello and welcome to What Da Math! In this video, we will talk about new various AGN objects such as Quasars, Blazars and Radio Galaxies and how to make them in Universe Sandbox 2. Enjoy and please subscribe. Buy the game here: http://store.steampowered.com/app/230290 Twitter: https://twitter.com/WhatDaMath Facebook: https://www.facebook.com/whatdamath Twitch: http://www.twitch.tv/whatdamath Patreon page: https://www.patreon.com/user?u=2318196&ty;=h Other videos here: https://www.youtube.com/playlist?list=PL9hNFus3sjE7jgrGJYkZeTpR7lnyVAk-x
These lectures give an in-depth observational overview of Active Galactic Nuclei (AGNs). Topics include the following: Introduction; AGN Basics; Finding AGNs; Terminology; The Black Hole Region; The Broad Line Region; Outflowing Winds; The Narrow Line Region; The Torus; Jets; and AGN Demography, Physics, and Ecology from X-ray Surveys. The total lecturing time is about 10.5 hours, and the lecturer is Prof. William N. Brandt (Penn State). There are two YouTube parts to these lectures. These lectures were presented from 2014 June 23-27 at the USTC Summer School on "Formation and Co-Evolution of Galaxies and Supermassive Black Holes" in Hefei, China. The lead organizer of the summer school was Prof. Yongquan Xue (USTC). See http://smbh2014.csp.escience.cn/dct/page/1 for details about the su...
A long time ago in a galaxy far, far away, something was feeding. That something was a supermassive black hole. When these things snack, they have the potential to outshine their entire host galaxy and it is this light that we can observe today. Termed Active Galactic Nuclei, they provide astronomers with evidence of extreme physical processes which are not yet fully understood. This will be a gentle introduction to the subject of AGN and how they have contributed to our understanding of the Universe. The lecture by Alastair Bruce was sponsored by the Institute of Physics in Scotland. It was recorded at Robert Gordon's College, Aberdeen, on Monday 5th October 2015.
Active galaxies pour out lots of energy, due to their central supermassive black holes gobbling down matter. Galaxies tend not to be loners, but instead exist in smaller groups and larger clusters. Our Milky Way is part of the Local Group, and will one day collide with the Andromeda galaxy. Clusters of galaxies also clump together to form superclusters, the largest structures in the Universe. In total, there are hundreds of billions of galaxies in the Universe. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Black Holes at the Center of Galaxies 2:26 Galaxies Are a Part of Small/Large Clusters 9:47 The Milky Way is Part of the Local Group 6:45 Galaxy Clusters Clump Together to Create Superclusters 11:03 Hundreds of Billion...
A team of astronomers using the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 (WFC3) have conducted a large survey to investigate the relationship between galaxies that have undergone mergers and the activity of the supermassive black holes at their cores. The team studied a large selection of galaxies with extremely luminous centres — known as active galactic nuclei (AGNs) — thought to be the result of large quantities of heated matter circling around and being consumed by a supermassive black hole. Whilst most galaxies are thought to host a supermassive black hole, only a small percentage of them are this luminous and fewer still go one step further and form what are known as relativistic jets. The two high-speed jets of plasma move almost with the speed of light and stream out i...
Most galaxies have at their cores a supermassive black hole hundreds of millions of times the mass of our Sun. They emit powerful ultraviolet radiation from the supermassive black hole at the core of the host galaxy. The most active of these galaxy cores are called quasars, where infalling material is heated to a point where a brilliant searchlight shines into deep space. The beam is produced by a disk of glowing, superheated gas encircling the black hole. Please join +Tony Darnell Dr.+Carol Christian and +Scott Lewis as they discuss some fascinating new observations of quasars made by the Hubble Space Telescope Read more here: http://hubblesite.org/newscenter/archive/releases/2015/13/ http://hubble25th.org #Hubble25 featured in Spaceport magazine: http://issuu.com/spaceportmagazine...
This simulation follows the collision of two spiral galaxies that harbor giant black holes. The collision merges the black holes and stirs up gas in both galaxies. The merged black hole gorges on the feast and lights up, forming an active galactic nucleus called a quasar and creating a "wind"" that blows away much of the galaxy's gas. "
Totally unscripted, unrehearsed, unprepared takes on the latest astronomy news stories from real scientists! Follow http://www.twitter.com/PaulMattSutter for more! Hosted by Paul Sutter (https://twitter.com/PaulMattSutter), Wayne Schlingman (https://twitter.com/stewardwildcat), Grace Calhoun (http://www.twitter.com/galacticgrace), and Anna Nierenberg (http://u.osu.edu/nierenberg.1/). Editing by Doug Dangler, OSU eLearning Program Manager. Useful links: Paul: http://www.pmsutter.com OSU: https://www.osu.edu Dept. of Physics: https://physics.osu.edu CCAPP: http://ccapp.osu.edu Dept. of Astronomy: https://astronomy.osu.edu Planetarium: https://planetarium.osu.edu College of Arts & Sciences: https://artsandsciences.osu.edu
This animation illustrates the anatomy of an active galactic nucleus powered by a supermassive black hole. The animation also shows how the viewing angle affects the appearance of the nucleus.
An "active galactic nucleus" is a compact region at the centre of a galaxy that has a much higher than normal luminosity over at least some portion – and possibly all – of the electromagnetic spectrum. Such excess emission has been observed in the radio, microwaves, infrared, optical, ultra-violet, X-ray and gamma ray wavebands. A galaxy hosting an AGN is called an "active galaxy", which is thought to be one of the candidates of high and ultra-high energy astroparticles " ". The radiation from AGN is believed to be a result of accretion of mass by a supermassive black hole at the centre of its host galaxy. AGN are the most luminous persistent sources of electromagnetic radiation in the universe, and as such can be used as a means of discovering distant objects; their evolution as a funct...
Hello and welcome to What Da Math! In this video, we will talk about new various AGN objects such as Quasars, Blazars and Radio Galaxies and how to make them in Universe Sandbox 2. Enjoy and please subscribe. Buy the game here: http://store.steampowered.com/app/230290 Twitter: https://twitter.com/WhatDaMath Facebook: https://www.facebook.com/whatdamath Twitch: http://www.twitch.tv/whatdamath Patreon page: https://www.patreon.com/user?u=2318196&ty;=h Other videos here: https://www.youtube.com/playlist?list=PL9hNFus3sjE7jgrGJYkZeTpR7lnyVAk-x
These lectures give an in-depth observational overview of Active Galactic Nuclei (AGNs). Topics include the following: Introduction; AGN Basics; Finding AGNs; Terminology; The Black Hole Region; The Broad Line Region; Outflowing Winds; The Narrow Line Region; The Torus; Jets; and AGN Demography, Physics, and Ecology from X-ray Surveys. The total lecturing time is about 10.5 hours, and the lecturer is Prof. William N. Brandt (Penn State). There are two YouTube parts to these lectures. These lectures were presented from 2014 June 23-27 at the USTC Summer School on "Formation and Co-Evolution of Galaxies and Supermassive Black Holes" in Hefei, China. The lead organizer of the summer school was Prof. Yongquan Xue (USTC). See http://smbh2014.csp.escience.cn/dct/page/1 for details about the su...
A long time ago in a galaxy far, far away, something was feeding. That something was a supermassive black hole. When these things snack, they have the potential to outshine their entire host galaxy and it is this light that we can observe today. Termed Active Galactic Nuclei, they provide astronomers with evidence of extreme physical processes which are not yet fully understood. This will be a gentle introduction to the subject of AGN and how they have contributed to our understanding of the Universe. The lecture by Alastair Bruce was sponsored by the Institute of Physics in Scotland. It was recorded at Robert Gordon's College, Aberdeen, on Monday 5th October 2015.
Most galaxies have at their cores a supermassive black hole hundreds of millions of times the mass of our Sun. They emit powerful ultraviolet radiation from the supermassive black hole at the core of the host galaxy. The most active of these galaxy cores are called quasars, where infalling material is heated to a point where a brilliant searchlight shines into deep space. The beam is produced by a disk of glowing, superheated gas encircling the black hole. Please join +Tony Darnell Dr.+Carol Christian and +Scott Lewis as they discuss some fascinating new observations of quasars made by the Hubble Space Telescope Read more here: http://hubblesite.org/newscenter/archive/releases/2015/13/ http://hubble25th.org #Hubble25 featured in Spaceport magazine: http://issuu.com/spaceportmagazine...
Ronen Plesser, Duke University, Introductory Astronomy. Week 10: Galaxies.
These lectures give an in-depth observational overview of Active Galactic Nuclei (AGNs). Topics include the following: Introduction; AGN Basics; Finding AGNs; Terminology; The Black Hole Region; The Broad Line Region; Outflowing Winds; The Narrow Line Region; The Torus; Jets; and AGN Demography, Physics, and Ecology from X-ray Surveys. The total lecturing time is about 10.5 hours, and the lecturer is Prof. William N. Brandt (Penn State). There are two YouTube parts to these lectures. These lectures were presented from 2014 June 23-27 at the USTC Summer School on "Formation and Co-Evolution of Galaxies and Supermassive Black Holes" in Hefei, China. The lead organizer of the summer school was Prof. Yongquan Xue (USTC). See http://smbh2014.csp.escience.cn/dct/page/1 for details about the su...
An active galactic nucleus (AGN) is a compact region at the centre of a galaxy that has a much higher than normal luminosity over at least some portion, and possibly all, of the electromagnetic spectrum. Such excess emission has been observed in the radio, microwaves, infrared, optical, ultra-violet, X-ray and gamma ray wavebands. A galaxy hosting an AGN is called an active galaxy. The radiation from AGN is believed to be a result of accretion of mass by a supermassive black hole at the centre of its host galaxy. AGN are the most luminous and persistent sources of electromagnetic radiation in the universe, and as such can be used as a means of discovering distant objects; their evolution as a function of cosmic time also puts constraints on models of the cosmos. This video is targeted to...
Extragalactic Relativistic Jets: Cause and Effect PROGRAM LINK: www.icts.res.in/program/ERG2015 DATES: Monday 12 Oct, 2015 - Tuesday 20 Oct, 2015 VENUE: Ramanujan Lecture Hall, ICTS Bangalore DESCRIPTION : Active Galactic Nuclei (AGN) are the luminous centers of galaxies that are believed to be powered by accretion of matter on to supermassive black holes. Bipolar outflows or jets that are launched from the accretion-disk black hole systems carry away angular momentum and impact the surrounding matter both inside and outside the host galaxies. Given the current computational power, AGN have become a test bed for general relativistic magnetohydrodynamics. AGN are sites of coalescing supermassive black holes, which are one of the primary science drivers of gravitational wave astronomy. ...
Daniel Proga University of Nevada, Las Vegas March 31, 2015 I review the physics of launching, acceleration, and propagation of radiation driven winds. I will consider two kinds of outflows powered by radiation emitted from the AGN central engine: (1) outflows driven from the innermost part of a black hole accretion disk and (2) outflows driven from a large-scale inflow. I discuss the relevance of both types of outflows to the so-called AGN feedback problem. However, as the AGN feedback should not be considered separately from the inner working of AGN, I also discuss the issue whether the properties of the same outflows are consistent with the observed gas properties in broad- and narrow-line regions of AGN. http://www.sns.ias.edu/~seminar/colloquia.shtml More videos on http://video.ias...