Results 131 to 140 of about 136,681 (287)
Using the upGREAT instrument on board the Stratospheric Observatory for Infrared Astronomy, we imaged [C ii ] 157.74 and [O i ] 63.18 μ m line emission from a bright photodissociation region (PDR) associated with an ionized bubble located in the Nessie ...
James M. Jackson +17 more
doaj +1 more source
Nitrogen hydrides in interstellar gas: Herschel/HIFI observations towards G10.6-0.4 (W31C) [PDF]
The HIFI instrument on board the Herschel Space Observatory has been used to observe interstellar nitrogen hydrides along the sight-line towards G10.6−0.4 in order to improve our understanding of the interstellar chemistry of nitrogen.
Bell, T. A. +6 more
core
Absorption Line Studies and the Distribution of Neutral Gas in the Local Interstellar Medium [PDF]
F. C. Bruhweiler
openalex +1 more source
Surveys of the Milky Way and Magellanic System in the λ21-cm line of atomic hydrogen
In the next three years, surveys of the Northern and Southern skies using focal plane arrays on aperture synthesis radio telescopes will lead to a breakthrough in our knowledge of the warm and cool atomic phases of the interstellar medium and their ...
Dickey J.M.
doaj +1 more source
Interstellar absorption lines in the spectrum of zeta Ophiuchi
The far-UV spectrum of Zeta Pup is surveyed as obtained from scans by Copernicus satellite detectors. Equivalent widths are tabulated for 147 lines from 35 different ions or isotopes of 19 elements in the direction of Zeta Pup. In addition, 52 unidentified absorption lines are listed whose narrow widths indicate an interstellar origin.
openaire +1 more source
Interstellar Absorption Lines in the Spectrum of the Starburst Galaxy NGC 1705 [PDF]
21 pages, AASTeX, 8 separate Postscript figure files, To appear in Astronomical Journal, September 1998 ...
openaire +2 more sources
Prospects for determining the cosmological helium-3 to helium-4 ratio via absorption-line studies of the local interstellar medium [PDF]
Mark Hurwitz, S. Bowyer
openalex +1 more source
The detection of circumstellar atomic hydrogen (H i ) via the 21 cm line remains a persistent challenge in planetary nebula (PN) studies, primarily due to contamination from ubiquitous interstellar H i 21 cm emission. In this paper, we report the results
Xu-Jia Ouyang +6 more
doaj +1 more source
Ultraviolet absorption line spectroscopy is a sensitive diagnostic for the properties of interstellar and circumgalactic gas. Down-the-barrel observations, where the absorption is measured against the galaxy itself, are commonly used to study feedback ...
R. Michael Jennings +15 more
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Quasar Winds Caught on Acceleration and Deceleration
We present an observational study of wind acceleration based on four low-ionization broad absorption line (BAL) quasars (J0136, J1238, J1259, and J1344).
Weimin Yi +7 more
doaj +1 more source

