Star formation in L 1199

Details Star formation in L 1199 Star formation in L 1199

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224...73k&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 73-76

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

Lynds 1199 is an extended dark cloud of moderate opacity in the upper Cepheus region. The B3V type star HD206135 illuminating the reflection nebula DG 175 is associated with this cloud. In this paper the nature of the cloud and its associated young stellar objects is studied on the basis of13CO data obtained with the 4 m millimeter wave telescope of Nagoya University, photographic observations taken with the 60/90 cm Schmidt telescope of Konkoly Observatory, as well as IRAS data.

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