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相关论文: Mapping the multiphase structure of H I in the Low…

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[ABRIDGED] We examine the velocity structure in the gas associated with \ion{H}{1} in the damped Ly$\alpha$ absorption system at redshift $z=1.7764$ towards the QSO $1331+170$ using 21cm data, optical and STIS spectra. We find at least two,…

宇宙学与河外天体物理 · 物理学 2015-05-20 R F Carswell , R A Jorgenson , A M Wolfe , M T Murphy

We present a detailed study of the HI 21cm absorption system at z=0.0912 towards the radio quasar B0738+313. The uncommonly narrow main absorption line and weak secondary line are resolved for the first time. In addition we find it…

天体物理学 · 物理学 2009-10-31 W. M. Lane , F. H. Briggs , A. Smette

Observations of Galactic H I gas for seven targeted regions at intermediate Galactic latitude are presented at 1' angular resolution using data from the DRAO Synthesis Telescope (ST) and the Green Bank Telescope (GBT). The DHIGLS data are…

We present methods and results from "21-cm Spectral Line Observations of Neutral Gas with the EVLA" (21-SPONGE), a large survey for Galactic neutral hydrogen (HI) absorption with the Karl G. Jansky Very Large Array (VLA). With the upgraded…

We present a detailed analysis of a H2-bearing metal-rich sub-damped Lyman-alpha system at zabs = 0.10115 towards the radio-loud quasar J0441-4313, at a projected separation of ~7.6 kpc from a star-forming galaxy. The H2, C I and Na I…

星系天体物理 · 物理学 2015-06-23 R. Dutta , R. Srianand , S. Muzahid , N. Gupta , E. Momjian , J. Charlton

The HI 21cm absorption optical depth and the N(HI) derived from Lya absorption can be combined to yield the spin temperature (Ts) of DLAs. Although Ts measurements exist for samples of DLAs with z <0.6 and z >1.7, the intermediate redshift…

宇宙学与河外天体物理 · 物理学 2015-06-05 Sara L. Ellison , Nissim Kanekar , J. Xavier Prochaska , Emmanuel Momjian , Gabor Worseck

We report the GMRT detection of HI 21cm absorption from the $z \sim 3.39$ damped Lyman-$\alpha$ absorber (DLA) towards PKS 0201+113, the highest redshift at which 21cm absorption has been detected in a DLA. The absorption is spread over…

天体物理学 · 物理学 2008-11-26 N. Kanekar , J. N. Chengalur , W. M. Lane

Tracing the transition between the diffuse atomic interstellar medium (ISM) and cold, dense gas is crucial for deciphering the star formation cycle in galaxies. Here we present MACH, a new survey of cold neutral hydrogen (HI) absorption at…

We investigate the physical processes occuring in the multiphase gas of a damped Ly\alpha system (DLA). We base our analysis on a high quality Keck HIRES spectrum of the QSO J1211+0422 in which a DLA is detected at z=2.377. There is little…

天体物理学 · 物理学 2009-11-13 N. Lehner , J. C. Howk , J. X. Prochaska , A. M. Wolfe

We develop a new method for spatially mapping a lower limit on the mass fraction of the cold neutral medium by analyzing the amplitude structure of $\hat T_b(k_v)$, the Fourier transform of $T_b(v)$, the spectrum of the brightness…

We present a statistical method for measuring the average HI spin temperature in distant galaxies using the expected detection yields from future wide-field 21cm absorption surveys. As a demonstrative case study we consider a simulated…

星系天体物理 · 物理学 2016-08-17 J. R. Allison , M. A. Zwaan , S. W. Duchesne , S. J. Curran

We present recent results from our searches of 21-cm absorption using GBT, GMRT, VLBA and WSRT to trace the evolution of cold gas in galaxies. Using ~130 sight lines with 21-cm absorption measurements, we find that within the measurement…

星系天体物理 · 物理学 2014-02-24 N. Gupta , R. Srianand , P. Petitjean , P. Noterdaeme , E. Momjian

We present a 21cm line HI self-absorption (HISA) survey of cold atomic gas within Galactic longitudes 75 to 146 degrees and latitudes -3 to +5 degrees. We identify HISA as spatially and spectrally confined dark HI features and extract it…

We report the detection of 21-cm and H2 absorption lines in the same DLA system (log N(HI)=21.36+-0.10) at zabs=3.17447 towards SDSSJ133724+315254 (z=3.174). We estimate the spin temperature of the gas to be, Ts~600 K, intermediate between…

宇宙学与河外天体物理 · 物理学 2015-05-18 R. Srianand , N. Gupta , P. Petitjean , P. Noterdaeme , C. Ledoux

Neutral hydrogen traces gravitational potentials. In the nearby universe, 21cm emission-line surveys show that the bulk of the HI resides in well-formed, optically-luminous galaxies. At high redshift, 21cm line absorption against background…

天体物理学 · 物理学 2007-05-23 F. H. Briggs

We report the discovery of two low redshift HI 21cm absorbers, one at z = 0.2212 towards the z_{em} = 0.630 quasar OI 363 (B0738+313), and the other at z = 0.3127 towards PKS B1127-145 (z_{em} = 1.187). Both were found during a survey of…

天体物理学 · 物理学 2009-10-30 W. Lane , A. Smette , F. Briggs , S. Rao , D. Turnshek , G. Meylan

Neutral hydrogen 21 cm transition is a useful tracer of the neutral interstellar medium. However, inferring physical condition from the observed 21 cm absorption and/or emission spectra is often not straightforward. One complication in…

星系天体物理 · 物理学 2021-01-13 Atanu Koley , Nirupam Roy

We present the results of a survey for 21-cm absorption in four never previously searched damped Lyman-alpha absorption systems (DLAs) with the Westerbork Synthesis Radio Telescope. We add our results to other recent studies in order to…

天体物理学 · 物理学 2009-11-13 S. J. Curran , P. Tzanavaris , Y. M. Pihlstroem , J. K. Webb

We report on the observed properties of the plasma revealed through high signal-to-noise (S/N) observations of 54 intervening O VI absorption systems containing 85 O VI and 133 H I components in a blind survey of 14 QSOs observed at ~18 km…

宇宙学与河外天体物理 · 物理学 2015-06-19 B. D. Savage , T. -S. Kim , B. P. Wakker , B. Keeney , J. M. Shull , J. T. Stocke , J. C. Green

Observations of the QSO HE 0153-4520 (z-em = 0.450) with the Cosmic Origins Spectrograph (COS) from 1134 to 1796 A with a resolution of ~17 km/s and signal-to- noise per resolution element of 20 to 40 are used to study a multi-phase partial…

宇宙学与河外天体物理 · 物理学 2015-05-27 B. D. Savage , A. Narayanan , N. Lehner , B. P. Wakker
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