Results 91 to 100 of about 34,908 (184)
Stars in galaxies form in giant molecular clouds that coalesce when the atomic hydrogen is converted into molecules. There are currently two dominant models for what property of the galactic disk determines its molecular fraction: either hydrostatic ...
Beck +63 more
core +1 more source
Modeling the gas-phase chemistry of the transitional disk around HD 141569A
Aims: The chemistry, distribution and mass of the gas in the transitional disk around the 5 Myr old B9.5 V star HD 141569A are constrained. Methods: A quasi 2-dimensional (2D) chemistry code for photon dominated regions (PDR) is used to calculate the ...
Augereau +38 more
core +4 more sources
Study of H i Turbulence in the SMC Using Multipoint Structure Functions
Turbulence in the interstellar medium (ISM) plays an important role in many physical processes, including forming stars and shaping complex ISM structures.
Bumhyun Lee +21 more
doaj +1 more source
X-ray spectroscopic observations and modeling of supernova remnants [PDF]
The X-ray observations of young remnants and their theoretical interpretation are described. A number of questions concerning the nature of the blast wave interaction with the interstellar gas and grains and of atomic processes in these hot plasmas are ...
Shull, J. M.
core +1 more source
The first results from the Herschel-HIFI mission
This paper contains a summary of the results from the first years of observations with the HIFI instrument onboard ESA's Herschel space observatory. The paper starts by outlining the goals and possibilities of far-infrared and submillimeter astronomy ...
van der Tak, Floris
core +2 more sources
n-Alkanes formed by methyl-methylene addition as a source of meteoritic aliphatics
Aliphatics prevail in asteroids, comets, meteorites and other bodies in our solar system. They are also found in the interstellar and circumstellar media both in gas-phase and in dust grains.
P. Merino +16 more
doaj +1 more source
H i Content of Group Galaxies from the FAST All Sky H i Survey
We investigate the atomic gas (H i ) content of galaxies in groups using early data from the Five-hundred-meter Aperture Spherical Radio Telescope (FAST) All Sky H i survey. Taking advantage of FAST’s blind, wide-area coverage and uniform sensitivity, we
Shulan Yan +5 more
doaj +1 more source
With new atomic-hydrogen (H i ) observations of FAST Extended Atlas of Selected Targets Survey (FEASTS), we present the first statistical comparison of H i morphology between observations and cosmological simulations, focusing on low-column-density (∼10 ^
Xuchen Lin +4 more
doaj +1 more source
The Impact of External Gas Accretion on the Distribution of H I Gas in Galaxies
Using the data from Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) and H i -MaNGA surveys, we build a sample of 37 gas–star misaligned galaxies with robust H i detections, which are believed to have undergone external gas accretion processes.
Qianhan Zhang +5 more
doaj +1 more source
Pervasive Cavity-rim Structure for Star Formation in Dwarf Irregular Galaxies
Unsharp-mask images of H I emission from 36 dwarf irregular (dIrr) galaxies illustrate star formation in dispersed clouds and on the rims of large cavities. The cavities can extend for a radial scale length and typically have circular or slightly sheared
Bruce G. Elmegreen, Deidre A. Hunter
doaj +1 more source

