Observations of H I absorption towards G74.9 + 1.2

Details Observations of H I absorption towards G74.9 + 1.2 Observations of H I absorption towards G74.9 + 1.2

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237..555g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, April 1, 1989, p. 555-559.

Astronomy and Astrophysics

Astronomy

14

Absorption Spectra, H I Regions, Stellar Spectra, Supernova Remnants, Radio Astronomy, Very Large Array (Vla)

Scientific paper

Observations with the VLA of neutral hydrogen absorption toward the filled-center supernova remnant G74.9 + 1.2 and the adjacent compact radio source 2013 + 370 are presented. These confirm the extragalactic nature of the compact source, and a distance of about 12 kpc for G74.9 + 1.2. From a continuum map, an upper limit is placed on the surface brightness of any shell around the remnant.

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