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The Bell Laboratories H I survey

The Astrophysical Journal Supplement SeriesPublished 1 March 1992
A. A. Stark, Charles F. Gammie, R. W. Wilson, John Bally, R. A. Linke, Carl Heiles
Citations774
SJR quartileQ1
SJR score3.34
SNIP2.28

Abstract

view Abstract Citations (1216) References (14) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Bell Laboratories H i Survey Stark, Antony A. ; Gammie, Charles F. ; Wilson, Robert W. ; Bally, John ; Linke, Richard A. ; Heiles, Carl ; Hurwitz, Mark Abstract Results of observations of the sky north of delta = -40 deg in the 21-cm line of atomic hydrogen are reported. The survey covers a velocity range of 654 km/s centered on the Galactic standard of rest, with 5.3-km/s wide filters. Calibration and reduction of the observations are described. The survey is presented as a series of images of the sky, each covering a 10-km/s wide velocity range. This survey is distinguished by its sensitivity to low surface brightness features (TA is approximately equal to 50 mK) and relative freedom from sidelobe contamination. High-velocity clouds are extracted and cataloged automatically. At the resolution of the survey, the lowest H I column density in the sky is 5.7 x 10 exp 19/cm. Publication: The Astrophysical Journal Supplement Series Pub Date: March 1992 DOI: 10.1086/191645 Bibcode: 1992ApJS...79...77S Keywords: H I Regions; Hydrogen Atoms; Interstellar Matter; Line Spectra; Radio Spectra; Sky Surveys (Astronomy); Emission Spectra; Interstellar Extinction; Milky Way Galaxy; Astronomy; ISM: GENERAL; RADIO LINES: ATOMIC; SURVEYS full text sources ADS | data products CDS (6) Related Materials (3) Catalog: 1993yCat.8010....0S Catalog: 1994yCat..20790077S Catalog: 1995yCat.8028....0S

Keywords

Earth and Planetary SciencesPhysics and Astronomy