The SGR A East H II complex at L = -0.02, B = -0.07 deg

Details The SGR A East H II complex at L = -0.02, B = -0.07 deg The SGR A East H II complex at L = -0.02, B = -0.07 deg

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.215p..69g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 215, July 15, 1985, p. 69P-73P.

Astronomy and Astrophysics

Astronomy

29

Molecular Clouds, Radio Sources (Astronomy), Stellar Evolution, Supernova Remnants, Continuous Spectra, H Alpha Line, H Ii Regions, Sagittarius Constellation, Very Large Array (Vla), Very Long Base Interferometry

Scientific paper

The four compact sources to the east of Sgr A East at l = -0°.02, b = -0°.07 have been observed by the Very Large Array with a resolution of 3 arcsec in the H76α line at 14.7 GHz. The sources are H II regions with velocities in the range 43 to 52 km s-1. These H II regions are almost certainly regions of recent star formation that can be associated with the 50 km s-1 molecular cloud.

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