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相关论文: The Nature of the Low-redshift Ly-alpha Clouds

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The low-redshift Ly-alpha forest of absorption lines provides a probe of large-scale baryonic structures in the intergalactic medium, some of which may be remnants of physical conditions set up during the epoch of galaxy formation. We…

天体物理学 · 物理学 2019-08-17 J. Michael Shull , Steven V. Penton , John T. Stocke

We present a study of the Ly\alpha forest at z<0.4 from which we conclude that at least 20% of the total baryons in the universe are located in the highly-ionized gas traced by broad Ly\alpha absorbers. The cool photoionized low-z…

天体物理学 · 物理学 2009-11-11 N. Lehner , B. D. Savage , P. Richter , K. R. Sembach , T. M. Tripp , B. P. Wakker

In Paper I of this series (astro-ph/9911117) we described observations of 15 extragalactic targets taken with the Hubble Space Telescope GHRS/G160M grating for studies of the low-z Lya forest. We reported the detection of 110 Lya absorbers…

天体物理学 · 物理学 2009-10-31 Steven V. Penton , J. Michael Shull , John T. Stocke

We present further observational results on our Lya-only absorber identification project at low and intermediate redshifts. We combine CFHT/MOS imaging and spectroscopic observations of 25 galaxies in the field of the quasar 3C286 (z_e =…

天体物理学 · 物理学 2007-05-23 V. Le Brun , J. Bergeron

We describe recent discoveries of low column density [N(HI) < 10^14.5 cm^-2] H I Ly-alpha absorbers made with the Hubble Space Telescope (HST), which have allowed us a first look at gas in local intergalactic space between us and the "Great…

天体物理学 · 物理学 2007-05-23 John T. Stocke

We have conducted pointed redshift surveys for galaxies in the direction of bright AGN whose HST far-UV spectra contain nearby (cz <~ 30,000 kms), low column density (12.5 <= log N_{HI} (cm s^{-2}) <= 14.5) Ly-alpha forest absorption…

天体物理学 · 物理学 2009-11-07 Kevin M. McLin , John T. Stocke , R. J. Weymann , Steven V. Penton , J. Micheal Shull

We report observations from the Hubble Space Telescope (HST) and the VLA on the galactic environment, metallicity, and D/H in strong low-redshift Lya absorption systems toward the bright BL Lac object PKS 2155-304. GHRS/G160M spectra at 20…

We present HST STIS/G140M spectra of 15 extragalactic targets, which we combine with GHRS/G160M data to examine the statistical properties of the low-z Ly-alpha forest. We evaluate the physical properties of these Ly-alpha absorbers and…

天体物理学 · 物理学 2008-11-26 Steven V. Penton , John T. Stocke , J. Michael Shull

To study the nature of low z Lya absorbers in the spectra of QSOs, we have obtained high signal-to-noise UV spectra of H 1821+643 (z = 0.297) and PG 1116+215 (z = 0.177) with the GHRS on the HST. The spectra have minimum S/N of 70-100 and 3…

天体物理学 · 物理学 2009-10-30 Todd M. Tripp , Blair D. Savage , Limin Lu

We present results from a spectroscopic and imaging survey of galaxies in the fields of quasars from the HST Quasar Absorption Line Key Project. The aim of this survey is to identify galaxies within 3.5' from the quasar sightline, to a…

天体物理学 · 物理学 2007-05-23 V. Le Brun , J. Bergeron , P. Boisse

We examine the Ly-alpha absorber population at z<0.3 detected in spectra of the QSOs PG0953+415 and H1821+643 taken with the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope. We compare their statistical properties to…

天体物理学 · 物理学 2009-11-06 Romeel Davé , Todd M. Tripp

We discuss the origin and physical nature of the Lya forest absorption systems as found in hydrodynamical simulations of the Intergalactic Medium in a standard Cold Dark Matter cosmology (Omega=1, H0=50 km/s/Mpc, sigma_8=0.7). The…

天体物理学 · 物理学 2009-10-26 Yu Zhang , Avery Meiksin , Peter Anninos , Michael L. Norman

In this paper, we use large-angle, nearby galaxy redshift surveys to investigate the relationship between the 81 low-redshift Lya absorbers in our HST/GHRS survey and galaxies, superclusters, and voids. In a subsample of 46 Lya absorbers…

天体物理学 · 物理学 2009-11-07 Steven V. Penton , John T. Stocke , J. Michael Shull

We present the target selection, observations, and data reduction and analysis process for a program aimed at discovering numerous, weak (equivalent width < 100 mA) Lya absorption lines in the local Universe (0.003 < z < 0.069). The purpose…

天体物理学 · 物理学 2016-08-30 Steven V. Penton , John T. Stocke , J. Michael Shull

We present intermediate resolution ($\sim3$ \AA ) spectra of the Ly$\alpha$ emission from 15 high redshift radio galaxies ($z>2$). Together with previously published spectra we analyze data for a sample of 18 objects. In 11 of the 18 radio…

天体物理学 · 物理学 2007-05-23 R. van Ojik , H. J. A. Röttgering , G. K. Miley , R. W. Hunstead

We present the results of a VLA and WSRT search for HI emission from the vicinity of seven nearby clouds, which were observed in Lya absorption with HST toward Mrk335, Mrk501 and PKS2155-304. We searched a volume of 40' x 40' x 1000 km/s.…

天体物理学 · 物理学 2009-10-28 J. H. van Gorkom , C. L. Carilli , John T. Stocke , Eric S. Perlman , J. Michael Shull

We report the detection, based on HST and Keck data, of two peculiar absorbers in the Ly-alpha forest of the quasar PKS 0454+039. These clouds, at redshifts z=0.6248 and 0.9315 respectively, display both MgII and FeII absorption lines in…

天体物理学 · 物理学 2007-05-23 V. Le Brun , C. W. Churchill

We present HST and FUSE observations of the intergalactic absorption toward PG1116+215 in the 900-3000 A spectral region. We detect 25 Ly-alpha absorbers at rest-frame equivalent widths W_r > 30 mA, yielding (dN/dz)_Ly-alpha = 154+/-18 over…

天体物理学 · 物理学 2009-11-10 Kenneth R. Sembach , Todd M. Tripp , Blair D. Savage , Philipp Richter

We present an analysis of the Ly-a forest toward 3C 273 from the Space Telescope Imaging Spectrograph at ~7 km/s resolution, along with re-processed data from the Far Ultraviolet Spectroscopic Explorer. The high UV flux of 3C 273 allows us…

宇宙学与河外天体物理 · 物理学 2015-05-18 G. M. Williger , R. F. Carswell , R. J. Weymann , E. B. Jenkins , K. R. Sembach , T. M. Tripp , R. Davé , L. Haberzettl , S. R. Heap

Spectra of the QSO pair Q0307-195A,B have been obtained in the Ly-alpha Forest (3660 - 3930 A) and C IV (4720 - 4850 A) regions with a FWHM resolution between 0.7 and 0.5 A. 46 lines have been detected in the spectrum of object A while 36…

天体物理学 · 物理学 2010-04-06 V. D'Odorico , S. Cristiani , S. D'Odorico , A. Fontana , E. Giallongo , P. Shaver
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