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Related papers: CO molecules in the shells of quasars 1556+3517 an…

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We have discovered two low-ionization broad absorption line quasars in programs to obtain optical spectra for radio-selected quasar candidates from the VLA FIRST Survey (Becker, White, & Helfand 1995). Both belong to the extremely rare…

A candidate radio-loud broad absorption line quasar (RLBAL) has been reported by Becker et al. (1997). We present JHK observations of this object and three other radio-detected BALs taken with the new Michigan-Dartmouth-MIT/Ohio…

Astrophysics · Physics 2009-10-30 Patrick B. Hall , Paul Martini , D. L. Depoy , Ian Gatley

We detected with the IRAM interferometer the lines of CO(4-3) and CO(9-8) from the recently-discovered broad absorption line quasar APM 08279+5255. The molecular lines are at a redshift of 3.911, which we take to be the true cosmological…

Astrophysics · Physics 2009-10-31 D. Downes , R. Neri , T. Wiklind , D. J. Wilner , P. Shaver

SDSS J083942.11+380526.3 is an Iron Low-ionization Broad Absorption Line (FeLoBAL) quasar at z = 2.3, and Aoki et al. (2006) recently found the presence of an H alpha absorption line in the broad H alpha emission line. Motivated by an idea…

We report the discovery of Balmer broad absorption lines (BALs) in the quasar LBQS 1206+1052 and present a detailed analysis of the peculiar absorption line spectrum. Besides Mg II $\lambda \lambda 2796, 2803$ doublet, BALs are also…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Tuo Ji , Tinggui Wang , Hongyan Zhou , Huiyuan Wang

HE 0141-3932 (zem = 1.80) is a bright blue radio-quite quasar with an unusually weak Ly-alpha emission line. Large redshift differences (Delta z = 0.05) are observed between high ionization and low ionization emission lines. Absorption…

Astrophysics · Physics 2009-11-10 D. Reimers , E. Janknecht , C. Fechner , I. I. Agafonova , S. A. Levshakov , S. Lopez

To date, the quasar 1556+3517 is the only radio loud Broad Absorption Line QSO (BALQSO; Becker et al. 1997). This prompted narrow band filter imaging observations in the range 4-15 micron with the ISO satellite. The source is clearly…

Astrophysics · Physics 2007-05-23 J. Clavel

We have obtained IRTF/SpeX spectra of eight moderate-redshift (z=0.7-2.4), radio-selected (log R*~0.4-1.9) broad absorption line (BAL) quasars. The spectra cover the rest-frame optical band. We compare the optical properties of these…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 J. C. Runnoe , R. Ganguly , M. S. Brotherton , M. A. DiPompeo

We present the detection of carbon monoxide molecules (CO) at z=1.6408 towards the quasar SDSSJ160457.50+220300.5 using the VLT Ultraviolet and Visual Echelle Spectrograph. CO absorption is detected in at least two components in the first…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 P. Noterdaeme , C. Ledoux , R. Srianand , P. Petitjean , S. Lopez

We present Keck spectropolarimetry of two rare low-ionization broad absorption line (BAL) QSOs, FIRST J084044.5+363328 and FIRST J155633.8+351758, that also exhibit narrow absorption lines from metastable excited levels of Fe II (``Iron…

Astrophysics · Physics 2015-06-24 M. S. Brotherton , Hien D. Tran , Wil van Breugel , Arjun Dey , Robert Antonucci

We have re-analyzed the X-ray spectra of the gravitational lensed high-redshift BAL QSO APM 08279+5255, observed with the XMM-Newton and Chandra observatories. Previous studies (Hasinger et al. 2002; Chartas et al. 2002) detected unusual,…

Astrophysics · Physics 2009-11-13 J. M. Ramírez

HE0141-3932 (zem=1.80) is a bright blue radio-quite quasar which reveals an emission line spectrum with an unusually weak Ly-alpha line. In addition, large redshift differences (Delta z=0.05) are observed between high ionization and low…

Astrophysics · Physics 2009-11-11 S. A. Levshakov , I. I. Agafonova , D. Reimers , C. Fechner , E. Janknecht , S. Lopez

The formation of low emission lines in quasars and active galactic nuclei is still an open issue. Aided by the organizing power of the 4D eigenvector 1 scheme, we review basic developments since the 1980s, devoting special attention to the…

Cosmology and Nongalactic Astrophysics · Physics 2013-11-08 Paola Marziani , Mary Loli Martinez-Aldama , Deborah Dultzin , Jack Sulentic

Absorption lines in front of distant quasars are quite rare in the millimeter domain. They can however bring a very useful and complementary information to emission lines. We report here the detection with NOEMA of CO(1-0) and CN(1-0) lines…

Astrophysics of Galaxies · Physics 2019-03-20 F. Combes , N. Gupta , G. I. G. Jozsa , E. Momjian

Recent XMM-Newton observations of the high-redshift, lensed, broad absorption line (BAL) quasi-stellar object APM 08279+5255, one of the most luminous objects in the universe, allowed the detection of a high column density absorber ($N_H…

Astrophysics · Physics 2009-11-07 G. Hasinger , N. Schartel , S. Komossa

We report the discovery of an unusual low--ionization broad absorption line quasar at z=1.776 which exhibits absorption lines from many excited states of Feii. This member of the rare class of 'FeLoBAL' quasars was serendipitously found in…

We have discovered a remarkable quasar, FIRST J101614.3+520916, whose optical spectrum shows unambiguous broad absorption features while its double-lobed radio morphology and luminosity clearly indicate a classic Fanaroff-Riley Type II…

Using the Karl G. Jansky Very Large Array (VLA), we have detected absorption lines due to carbon-monoxide, CO(J=0-1), and the cyano radical, CN(N=0-1), associated with radio galaxy B2 0902+34 at redshift z=3.4. The detection of…

We report the discovery of X-ray broad absorption lines (BALs) from the BALQSO APM 08279+5255 originating from material moving at relativistic velocities with respect to the central source. The large flux magnification by a factor of ~ 100…

Astrophysics · Physics 2009-11-07 G. Chartas , W. N. Brandt , S. C. Gallagher , G. P. Garmire

We present the analysis of multi-wavelength observations of bright quasar HS1603+3820: the optical data taken with the MMT and Keck telescopes, and X-ray data obtained with the Chandra X-ray Observatory. The optical spectra contain a very…

Astrophysics · Physics 2009-06-25 A. Dobrzycki , M. Nikolajuk , J. Bechtold , H. Ebeling , B. Czerny , A. Rozanska
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