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gas agn published presentations and documents on DocSlides.

AGN downsizing
AGN downsizing
by tawny-fly
は階層的銀河形成論で説明. できる...
Physical Conditions in the ISM
Physical Conditions in the ISM
by backbays
Lisa Kewley. Australian National University. Thank...
Feeding the monster: fueling mechanisms of AGN
Feeding the monster: fueling mechanisms of AGN
by pasty-toler
Ioana. . Duţ. an. Advisors: Peter Biermann &...
MOLECULAR GAS IN THE CORES OF AGN
MOLECULAR GAS IN THE CORES OF AGN
by cheryl-pisano
Violette Impellizzeri (NRAO). Alan Roy (. MPIfR. ...
Color Magnitude Diagram
Color Magnitude Diagram
by alida-meadow
VG. So we want a color magnitude diagram for AGN ...
Tracing HI gas within dust-reddened quasars with
Tracing HI gas within dust-reddened quasars with
by liane-varnes
ASKAP. Marcin Glowacki. Supervisors: Elaine Sadle...
Key points
Key points
by myesha-ticknor
:. Active Galactic Nuclei: powerful energy source...
Microphysics and X-ray Spectra of AGN Outflows
Microphysics and X-ray Spectra of AGN Outflows
by cheryl-pisano
T. Kallman NASA/GSFC. Line emission efficiency ac...
Connecting Warm H
Connecting Warm H
by natalia-silvester
2. Emission and Active Transformation within Com...
Black Hole Fueling
Black Hole Fueling
by faustina-dinatale
Image from ESO. Accretion to Supermassive Black H...
A Critical Role for Viscosity in the Radio Mode AGN Feedbac
A Critical Role for Viscosity in the Radio Mode AGN Feedbac
by giovanna-bartolotta
Paul Nulsen. Harvard-Smithsonian Center for Astro...
BULGE FRACTION AND DISTRIBUTION OF STAR FORMATION IN SAMI G
BULGE FRACTION AND DISTRIBUTION OF STAR FORMATION IN SAMI G
by lindy-dunigan
Greg Goldstein. PhD student, . Dept. of Physics ...
Radiation Pressure Confinement
Radiation Pressure Confinement
by luanne-stotts
and its Implications for the Coupling of a Quasar...
Bacterial infections of the Respiratory Tract 1
Bacterial infections of the Respiratory Tract 1
by vivian
By: Nader . Alaridah. MD, PhD. STREPTOCOCCUS. The...
Many galaxies have powerful energy sources in their nuclei
Many galaxies have powerful energy sources in their nuclei
by celsa-spraggs
These are called . active. . galaxies. .. . Act...
Active Galaxies
Active Galaxies
by debby-jeon
Most of the power of galaxies come from the stars...
Cloudy Simulations AGN Warm Absorbers Science Goals Roughly of Seyfert nuclei and perhaps of quasars have Xray spectra that are suppressed by continuous absorption
Cloudy Simulations AGN Warm Absorbers Science Goals Roughly of Seyfert nuclei and perhaps of quasars have Xray spectra that are suppressed by continuous absorption
by myesha-ticknor
The Xray absorbing gas is often called a warm abs...
Radio Mode Feedback in Giant Elliptical Galaxies
Radio Mode Feedback in Giant Elliptical Galaxies
by celsa-spraggs
Paul . Nulsen. (. CfA. ), Christine Jones (. CfA...
A bit of (my) history
A bit of (my) history
by danika-pritchard
My main PhD simulations were performed on COSMOS ...
Radio Mode Feedback in Giant Elliptical Galaxies
Radio Mode Feedback in Giant Elliptical Galaxies
by faustina-dinatale
Paul . Nulsen. (. CfA. ), Christine Jones (. CfA...