Results 101 to 110 of about 34,658 (198)
Analysis of ultraviolet spectrophotometric data from Copernicus [PDF]
Ultraviolet spectral data from the OAO 3 satellite are being used to study interstellar absorption lines and stellar and circumstellar lines in hot stars.
Snow, T. P., Jr.
core +1 more source
Reaction Networks For Interstellar Chemical Modelling: Improvements and Challenges
We survey the current situation regarding chemical modelling of the synthesis of molecules in the interstellar medium. The present state of knowledge concerning the rate coefficients and their uncertainties for the major gas-phase processes -- ion ...
Agundez, M. +12 more
core +3 more sources
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
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
Gas phase atomic metals in the circumstellar envelope of IRC+10216
We report the results of a search for gas phase atomic metals in the circumstellar envelope of the AGB carbon star IRC+10216. The search was made using high resolution (R=50000) optical absorption spectroscopy of a backgound star that probes the envelope
Chaffee +46 more
core +1 more source
Extraterrestrial Effects of Cosmic Rays [PDF]
So far only interactions of cosmic rays with terrestrial matter have been investigated. If cosmic rays are present in interstellar and intergalactic space, they produce physical changes on extraterrestrial objects also.
Zwicky, F.
core
Interstellar Neutral Hydrogen in the Heliosphere: New Horizons Observations in the Context of Models
Interstellar neutral (ISN) hydrogen is the most abundant species in the outer heliosheath and the very local interstellar medium (VLISM). Charge-exchange collisions in the outer heliosheath result in filtration, reducing the ISN hydrogen density inside ...
P. Swaczyna +14 more
doaj +1 more source
Mapping Galactic Dust Emission and Extinction with H I, H II, and H2
Neutral hydrogen (H i ) emission closely traces the dust column density at high Galactic latitudes and is thus a powerful tool for predicting dust extinction. However, the relation between H i column density N _HI and high-latitude dust emission observed
Yun-Ting Cheng +3 more
doaj +1 more source
Strottner–Drechsler–Sainty Object 1 (SDSO1) is a faint [O iii ] emission nebula spanning 1 $\mathop{.}\limits^{^\circ }5$ , discovered southeast of M31.
Tiantian Liang +18 more
doaj +1 more source
Forbidden transition properties in the ground-state configurations of singly ionized noble gas atoms for stellar and interstellar media [PDF]
D. K. Nandy, B. K. Sahoo
openaire +1 more source

