The young cluster NGC 5367 and A1353-40

Details The young cluster NGC 5367 and A1353-40 The young cluster NGC 5367 and A1353-40

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.180..709w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 180, Sept. 1977, p. 709-715.

Astronomy and Astrophysics

Astronomy

17

Binary Stars, Interstellar Matter, Nebulae, Star Clusters, Supernovae, X Ray Sources, Astronomical Spectroscopy, Balmer Series, Stellar Envelopes, Stellar Evolution, Stellar Spectrophotometry

Scientific paper

The sparse young cluster embedded in and illuminating NGC 5367 in the head of Cometary Globule 12 is shown to suffer about 1 magnitude of visual extinction in the cloud and to be about 630 pc away. Infrared photometry and scanner spectroscopy of the two most luminous members, comprising the double h 4636, indicate that one component is surrounded by a circumstellar shell producing Balmer line emission and thermal reradiation by grains. The proposed identification of NGC 5367 with the transient X-ray source A1353-40 is not favored. It is suggested that NGC 5367 lies on an H I loop and that star formation in it was induced by a supernova explosion near galactic longitude 320 deg, latitude 30 deg, about 10 million years ago.

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