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相关论文: HI-selected Galaxies as a probe of Quasar Absorpti…

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Using the Atacama Large Millimeter/sub-millimeter Array, we have detected CO(3-2) line and far-infrared continuum emission from a galaxy associated with a high-metallicity ([M/H] = -0.27) damped Ly-alpha absorber (DLA) at z =2.19289. The…

In a 21 cm neutral hydrogen survey of approximately 55 sq deg out to a redshift of cz=8340 km/s, we have identified 75 extragalactic HI sources. These objects comprise a well-defined sample of extragalactic sources chosen by means that are…

天体物理学 · 物理学 2009-10-31 John G. Spitzak , Stephen E. Schneider

Galaxy disks are shown to contain a significant population of atomic clouds of 100pc linear size which are self-opaque in the 21cm transition. These objects have HI column densities as high as 10^23 and contribute to a global opacity…

宇宙学与河外天体物理 · 物理学 2015-06-04 Robert Braun

In this paper we present Monte-Carlo simulations of Lyman alpha absorption systems which originate in galactic haloes, galaxy discs and dark matter (DM) satellites around big central haloes. It is found that for strong Lyman alpha…

天体物理学 · 物理学 2009-10-31 W. P. Lin , G. Boerner , H. J. Mo

The formation mechanism of high-concentration dwarf galaxies is still a mystery. We perform a comparative study of the intrinsic shape of nearby low-mass galaxies with different stellar concentration. The intrinsic shape is parameterized by…

星系天体物理 · 物理学 2023-09-12 Lijun Chen , Hong-Xin Zhang , Zesen Lin , Guangwen Chen , Bojun Tao , Zhixiong Liang , Zheyu Lin , Xu Kong

We present a method to measure the the oblateness parameter q of the dark matter halos of gas rich galaxies that have extended HI disks. We have applied our model to a sample of 20 nearby galaxies that are gas rich and close to face-on, of…

星系天体物理 · 物理学 2026-01-14 Mousumi Das , Roger Ianjamasimanana , Stacy McGaugh , James Schombert , K. S. Dwarakanath

Using a spectral stacking technique we searched for the average \lya emission from high-z Damped \lya (DLA) galaxies detected in the Sloan Digital Sky Survey QSO spectra. We used a sample of 341 DLAs of mean redshift <z>= 2.86 and log N(HI)…

宇宙学与河外天体物理 · 物理学 2015-05-19 H. Rahmani , R. Srianand , P. Noterdaeme , P. Petitjean

Deep wide spectral line surveys with the Square Kilometre Array (SKA) will expand the cosmic frontiers of neutral atomic hydrogen (HI) in galaxies. However, at cosmologically significant redshifts ($z \gtrsim 0.5$), detections will…

星系天体物理 · 物理学 2025-02-12 Charissa Button , Roger Deane

We interpret observations of intergalactic low ionisation metal absorption systems at redshifts z $\gtrsim$5 in terms of pressure-confined clouds. We find clouds confined by the expected pressure of galactic haloes with masses $11<\log…

宇宙学与河外天体物理 · 物理学 2021-01-27 Teresita Suarez , Avery Meiksin

We present a demographic analysis of integrated star formation and gas properties for a sample of galaxies representative of the overall population at z~0. This research was undertaken in order to characterise the nature of star formation…

宇宙学与河外天体物理 · 物理学 2015-05-13 M. S. Bothwell , R. C. Kennicutt , J. C. Lee

We report coincident damped Lyman alpha (DLA) and sub-DLA absorption at z = 2.66 and z = 2.94 towards the z ~ 3 13.8 arcsecond separation binary quasar SDSS 1116+4118 AB. At the redshifts of the absorbers, this angular separation…

天体物理学 · 物理学 2009-06-23 Sara L. Ellison , Joseph F. Hennawi , Crystal L. Martin , Jesper Sommer-Larsen

Details of processes through which galaxies convert their gas into stars need to be studied in order to obtain a complete picture of galaxy formation. One way to tackle these phenomena is to relate the HI gas and the stars in galaxies.…

宇宙学与河外天体物理 · 物理学 2015-05-19 Celine Peroux , Nicolas Bouche , Varsha P. Kulkarni , Donald G. York , Giovanni Vladilo

We present the first results from a survey of SDSS quasars selected for strong H I damped Lyman-{\alpha} (DLA) absorption with corresponding low equivalent width absorption from strong low-ion transitions (e.g. C II {\lambda}1334 and Si II…

宇宙学与河外天体物理 · 物理学 2010-06-22 Bryan E. Penprase , J. Xavier Prochaska , Wallace L. W. Sargent , Irene Toro Martinez , Daniel J. Beeler

We probe the physical conditions in high redshift galaxies, specifically, the Damped Lyman-alpha Systems (DLAs) using neutral carbon (CI) fine structure lines and molecular hydrogen (H2). We report five new detections of CI and analyze the…

宇宙学与河外天体物理 · 物理学 2015-05-19 Regina A. Jorgenson , Arthur M. Wolfe , J. Xavier Prochaska

We analyze the properties of a rare population, the strongly bulge-dominated early-type galaxies (referred to as sBDEs) with significant HI gas, using the databases from the FAST All Sky HI survey (FASHI) and the Arecibo Legacy Fast ALFA…

星系天体物理 · 物理学 2024-08-09 Fujia Li , Enci Wang , Ming Zhu , Yingjie Peng , Jing Wang , Chuanpeng Zhang , Zesen Lin , Yu Rong , Hongxin Zhang , Xu Kong

We present the results from VLT/X-shooter spectroscopic observations of 11 extremely strong intervening damped Lyman-alpha absorbers (ESDLAs) initially selected as high N(Hi) (i.e.>=5x10^21 cm-2) candidates from the Sloan Digital Sky Survey…

星系天体物理 · 物理学 2020-01-22 A. Ranjan , P. Noterdaeme , J. -K. Krogager , P. Petitjean , R. Srianand , S. A. Balashev , N. Gupta , C. Ledoux

Hydro cosmological simulations reveal that massive galaxies at high redshift are fed by long narrow streams of merging galaxies and a smoother component of cold gas. We post-process seven high-resolution simulated galaxies with radiative…

宇宙学与河外天体物理 · 物理学 2015-05-27 Michele Fumagalli , J. Xavier Prochaska , Daniel Kasen , Avishai Dekel , Daniel Ceverino , Joel R. Primack

Recently, the number of detected galaxy counterparts of z > 2 Damped Lyman-alpha Absorbers in QSO spectra has increased substantially so that we today have a sample of 10 detections. M{\o}ller et al. in 2004 made the prediction, based on a…

宇宙学与河外天体物理 · 物理学 2015-06-04 J. -K. Krogager , J. P. U. Fynbo , P. Møller , C. Ledoux , P. Noterdaeme , L. Christensen , B. Milvang-Jensen , M. Sparre

We present the results of our automatic search for proximate damped Ly$\alpha$ absorption (PDLA) systems in the quasar spectra from the Sloan Digital Sky Survey Data Release 12. We constrain our search to those PDLAs lying within 1500 km…

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