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Trace gas phosphine points to volcanic activity on Venus(图)     微量气体  磷化氢  金星  火山活动       font style='font-size:12px;'> 2023/5/24
Scientists last autumn revealed that the gas phosphine was found in trace amounts in Venus’ upper atmosphere. That discovery promised the slim possibility that phosphine serves as a biological signatu...
Astronomers studying a cluster of still-forming protogalaxies seen as they were more than 10 billion years ago have found that a giant galaxy in the center of the cluster is forming from a surprisingl...
Tsunami of Stars and Gas Produces Dazzling Eye-shaped Feature in Galaxy     Tsunami  Stars  Gas  Dazzling Eye-shaped  Galaxy       font style='font-size:12px;'> 2016/11/29
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have discovered a tsunami of stars and gas that is crashing midway through the disk of a spiral galaxy known as IC 2163. This ...
How do galaxies get their gas?     these theoretical  observational transitions       font style='font-size:12px;'> 2014/12/24
We examine the temperature history of gas accreted by forming galaxies in smoothed particle hydrodynamics simulations. About half of the gas follows the track expected in the conventional picture of g...
We report new K-band, radio continuum, and CO (1-0) imaging observations and 850 μm photometric observations of PDS 456, the most luminous QSO in the local universe (z < 0.3). The 06 resolution K-band...
X-Raying A2125: A Large-Scale Hierarchical Complex of Galaxies and Hot Gas     Abell 2125  X-rays       font style='font-size:12px;'> 2014/12/24
We present an 82 ks Chandra ACIS-I observation of a large-scale hierarchical complex, which consists of various clusters/groups of galaxies and low surface brightness X-ray emission at z = 0.247. This...
Dense, Ionized, and Neutral Gas Surrounding Sagittarius A*     center  nuclei       font style='font-size:12px;'> 2014/12/24
We present high-resolution H41α hydrogen recombination line observations of the 12 (3 pc) region surrounding Sagittarius A* (Sgr A*) at 92 GHz using the Millimeter Array at the Owens Valley Radio Obse...
We investigate the detailed response of gas to the formation of transient and long-lived dynamical structures induced in the early stages of a disk-disk collision and identify observational signatures...
High-Density Molecular Gas in the Infrared-bright Galaxy System VV 114     kinematics and dynamics  VV 114       font style='font-size:12px;'> 2014/12/24
The new high-resolution CO (3-2) interferometric map of the IR-bright interacting galaxy system VV 114 observed with the Submillimeter Array reveals a substantial amount of warm and dense gas in the I...
X-ray absorption lines of highly ionized species such as O VII at about zero redshift have been firmly detected in the spectra of several active galactic nuclei. However, the location of the absorbing...
Extra-planar Diffuse Hot Gas Around Normal Disk Galaxies     Hot Gas   Galaxies       font style='font-size:12px;'> 2014/12/24
I review results from Chandra observations of nearby normal edge-on galaxies (Sd to Sa types). These galaxies have a broad range of star formation rate, but none of them is dominated by a nuclear star...
How do galaxies get their gas?     formation  evolution       font style='font-size:12px;'> 2014/12/24
We examine the temperature history of gas accreted by forming galaxies in smoothed particle hydrodynamics simulations. About half of the gas follows the track expected in the conventional picture of g...
Atomic and Molecular Gas in Colliding Galaxy Systems. I. The Data     NGC 7253/54  NGC 4567/68       font style='font-size:12px;'> 2014/12/24
We present H I and CO (1-0) interferometric observations of 10 comparable-mass interacting systems obtained at the Very Large Array (VLA) and the Owens Valley Radio Observatory (OVRO) millimeter array...
We present 12CO(J = 1 → 0) observations of the high-redshift quasi-stellar objects (QSOs) BR 1202-0725 (z = 4.69), PSS J2322+1944 (z = 4.12), and APM 08279+5255 (z = 3.91) using the NRAO Green Bank Te...
The Nonisothermality and Extent of Galactic Diffuse Hot Gas toward Markarian 421     ISM  Mrk 421       font style='font-size:12px;'> 2014/12/23
Diffuse hot gas can be traced effectively by its X-ray absorption and emission. We present a joint analysis of these tracers to characterize the spatial and temperature distributions of the Galactic h...

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