Young and Explosive BAL QSOs (at low and high redshifts) (original) (raw)
Infrared mergers and infrared quasi-stellar objects with galactic winds - III. Mrk 231: an exploding young quasi-stellar object with composite outflow/broad absorption lines (and multiple expanding superbubbles)
Roberto Terlevich
Monthly Notices of the Royal Astronomical Society, 2005
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GEMINI 3D spectroscopy of BAL + IR + Fe ii QSOs - I. Decoupling the BAL, QSO, starburst, NLR, supergiant bubbles and galactic wind in Mrk 231
Sebastián F. Sánchez Sánchez
Monthly Notices of the Royal Astronomical Society, 2009
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Gemini 3D spectroscopy of BAL+IR+Fe ii QSOs - II. IRAS 04505−2958, an explosive QSO with hypershells and a new scenario for galaxy formation and galaxy end phase
DAVID C Merlo
Monthly Notices of the Royal Astronomical Society, 2009
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GEMINI 3D spectroscopy of BAL+IR+Fe II QSOs: II. IRAS 04505-2958 an explosive QSO with hypershell and a new scenario for galaxy formation and galaxy end
Roberto Terlevich
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Gemini 3D-Spectroscopy of IRAS 17002+5153 and IRAS 07598+6508: Evidence of Two New Exploding BAL + IR + Fe ii QSOs
Roberto Terlevich
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Deep GEMINI GMOS-IFU spectroscopy of BAL QSOs: I. Decoupling the BAL, QSO, starburst, NLR, supergiant bubbles and galactic wind in Mrk 231
Roberto Terlevich
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Star-formation at z= 4.7 in the environment of the QSO BR1202-07
Patrick Petitjean
Arxiv preprint astro-ph/ …, 1998
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Near-infrared spectroscopy of extreme BAL QSOs from the QUBRICS bright quasar survey
Valentina D'Odorico
Monthly Notices of the Royal Astronomical Society, 2021
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Red Quasars and Quasar Evolution: The Case of BAL QSO FIRST J155633.8+351758
Mike Brotherton
The Astronomical Journal, 2000
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Very High Density Clumps and Outflowing Winds in QSO Broad-Line Regions
Belinda Wilkes
The Astrophysical Journal, 1996
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The parsec-scale structure of radio-loud broad absorption line quasars
F. Montenegro-Montes, D. Dallacasa
Astronomy & Astrophysics, 2013
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Properties of the molecular gas in a starbursting QSO at z = 1.83 in the COSMOS field
Christian Henkel
Astronomy and Astrophysics, 2008
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The emission-line properties of the QSO population at Z approximately 2
Paul Francis
The Astronomical Journal, 1994
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Herschel -ATLAS: the far-infrared properties and star formation rates of broad absorption line quasi-stellar objects
A. Cava
Monthly Notices of the Royal Astronomical Society, 2012
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High-redshift QSOs in the GOODS
Ray Lucas
Multiwavelength Mapping of Galaxy Formation and Evolution, 2005
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Evidence Against BALS in the X-ray Bright QSO PG1416-129
Paul Green
Eprint Arxiv Astro Ph 9702207, 1997
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Extreme BAL Quasars from the Sloan Digital Sky Survey
Michael Strauss
Arxiv preprint astro-ph/ …, 2001
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Low Redshift BAL QSOs in the Eigenvector 1 Context
Deborah Dultzin Kessler
arXiv (Cornell University), 2005
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Star formation in QSO host galaxies
Mike Brotherton
New Astronomy Reviews, 2006
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The Hamburg/ESO survey for bright QSOs. III. A large flux-limited sample of QSOs
Volker Beckmann
Astronomy & Astrophysics, 2000
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High‐Redshift QSOs in the SWIRE Survey and thez∼3 QSO Luminosity Function
Thomas Babbedge
The Astrophysical Journal, 2008
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DIRECT EVIDENCE FOR TERMINATION OF OBSCURED STAR FORMATION BY RADIATIVELY DRIVEN OUTFLOWS IN REDDENED QSOs
Jose Afonso
The Astrophysical Journal, 2012
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A Chandra Survey of Broad Absorption Line Quasars
Paul Green
The Astrophysical Journal, 2001
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The nature of G52.381-0.849 and G56.240-0.345: young stellar objects associated with extended mid-infrared emission?
Gerardo Ramos-Larios
Monthly Notices of the Royal Astronomical Society, 2010
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HST observations of the QSO pair Q1026-0045A,B
Marc Remy
Astronomy & Astrophysics, 1998
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The Role of Exploding QSOs in Explosive Models of Evolution, Formation and End of Galaxies
Roberto Terlevich
2007
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On the nature of outflows in intermediate-mass protostars: a case study of IRAS 20050+2720
Josep Miquel Girart
Astronomy & Astrophysics, 2008
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The low-mass YSO CB230-A: investigating the protostar and its jet with NIR spectroscopy and Spitzer observations
Luca Di Fabrizio
Astronomy and Astrophysics, 2008
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Mid‐Infrared Spitzer Spectra of X‐Ray–Selected Type 2 QSOs: QSO2s Are Not Ultraluminous Infrared Galaxies
L. Taconi
The Astrophysical Journal, 2006
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