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Rapid-fire fast radio burst shows hot space between galaxies(图)     快速射电爆发  星系  热空间       font style='font-size:12px;'> 2023/5/22
A rare and persistent rapid-fire fast radio burst source – sending out an occasional and informative cosmic ping from more than 3.5 billion light years away – now helps to reveal the secrets of the br...
最近,南京大学天文与空间科学学院行星课题组与北京大学科维理天文研究所等单位合作利用国家天文台的郭守敬望远镜(LAMOST)发现了一类新的太阳系外行星族群—热海星(Hoptunes)。相关研究论文(标题为LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of star...
Yale researchers have identified 60 potential new “hot Jupiters” — highly irradiated worlds that glow like coals on a barbecue grill and are found orbiting only 1% of Sun-like stars.Hot Jupiters const...
Earth-Space Telescope System Produces Hot Surprise     Earth-Space Telescope System  Hot Surprise       font style='font-size:12px;'> 2016/4/13
Astronomers using an orbiting radio telescope in conjunction with four ground-based radio telescopes have achieved the highest resolution, or ability to discern fine detail, of any astronomical observ...
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...
X-Ray Absorption Line Spectroscopy of the Galactic Hot Interstellar Medium     Cyg X–2  V801 Ara       font style='font-size:12px;'> 2014/12/24
We present an X-ray absorption line spectroscopic study of the large-scale hot interstellar medium (HISM) in the Galaxy. We detect Ne IX Kα absorption lines in the Chandra grating spectra of seven Gal...
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...
Most supernovae are expected to explode in low-density hot media, particularly in galactic bulges and elliptical galaxies. The remnants of such supernovae, although difficult to detect individually, c...
The iron depletion level and the gas-phase iron abundance in the hot (~106 K) interstellar medium (ISM) are critical to our understanding of its energy balance as well as the thermal sputtering, cooli...
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...
Hot Gaseous Halos of Nearby Disk Galaxies     Disk Galaxies  Hot Gaseous Halos       font style='font-size:12px;'> 2014/12/23
I review studies of the hot gaseous medium in and around nearby normal disk galaxies, including the Milky Way. This medium represents a reservoir of materials required for lasting star formation, a de...
Chandra Detection of Diffuse Hot Gas in and around the M31 Bulge     spiral  general       font style='font-size:12px;'> 2014/12/23
We report the detection of diffuse hot gas in M31, using archival Chandra observations that allow us to map out a 30' × 30' field (covering a galactocentric radius up to 4.5 kpc) and to detect sources...
Limits on Hot Galactic Halo Gas from X-Ray Absorption Lines     4U 1957+11  Mrk 421  LMC X–3       font style='font-size:12px;'> 2014/12/23
Although the existence of large-scale hot gaseous halos around massive disk galaxies has been theorized for a long time, there is yet very little observational evidence. We report the Chandra and XMM-...
We study the edge-on galaxy NGC 5775, utilizing a 58.2 ks Chandra ACIS-S observation together with complementary Hubble Space Telescope (HST) ACS, Spitzer IRAC and other multi-wavelength data sets. Th...

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