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Markarian 231
NUSTAR REVEALS an INTRINSICALLY X-RAY WEAK BROAD ABSORPTION LINE QUASAR in the ULTRALUMINOUS INFRARED GALAXY MARKARIAN 231 Stacy H
Explosion Shutting Down a Galactic Party: Physicists
Herschel-PACS Spectroscopic Diagnostics of Local Ulirgs
A Multimessenger View of Galaxies and Quasars from Now to Mid-Century M
Quasar's Belch Solves Longstanding Mystery (W/ Video) 24 February 2011, by Peter Michaud
A Ks–Band Selected, Multi–Wavelength Survey for Quasars In
The Competing Depleters of Gas in the Quasar Markarian
From the Hot, Nuclear, Ultra-Fast Wind to the Galaxy-Scale, Molecular Outflow
I. Personal Information
The Multi-Phase Winds of Markarian 231: from the Hot, Nuclear, Ultra-Fast Wind to the Galaxy-Scale, Molecular Outflow?
Felipe Ardila
The “Big Question” of Cosmology Cosmology and Religion In
A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
The WISSH Quasars Project IV
197 7MNRAS.178. .451B Mon. Not. R. Astr. Soc. (1977
Morphology and Spectroscopy of Markarian 231
Research Paper
AGN Feedback on Molecular Gas Reservoirs in Quasars at Z ~
Top View
Euclid Imaging Consortium Science Book
Arxiv:2009.03341V1 [Astro-Ph.GA] 7 Sep 2020
Galaxies Through Space and Time Contents INTRODUCTION 4
High Spatial Resolution HST/NICMOS Observations Of
1974Apj. . .192. .581K the Astrophysical Journal, 192:581-589
Astronomers Glimpse Birth of a Quasar
Katherine Alatalo, Ph.D
O B E R N G S U M M A
Arxiv:Astro-Ph/9911045V1 3 Nov 1999
AGN Wind Scaling Relations and the Co-Evolution of Black Holes and Galaxies F
Press Release
An ALMA/NOEMA Survey of the Molecular Gas Properties of High-Redshift Star-Forming Galaxies.', Monthly Notices of the Royal Astronomical Society, 501 (3)
Giant Black Holes Lurking in Survey Data 8 October 2012
Visually Observing Quasars by Ian Wheelband and Blake Nancarrow
AGN Wind Scaling Relations and the Co-Evolution of Black Holes and Galaxies
171 Hidden Pairs of Supermassive Black Holes
PUBLIC OPEN EVENING Surface of Betelgeuse Observed by ESO
Studying the Large Scale Structure and Interstellar Medium of Galaxies
Thesis Are Based on OH Emitters and on One Particular OH Absorber, Which Also Shows H2O Megamaser Emission
(A-Level) : Paper 3 Section B Option a Astrophysics