Cepheus flare molecular clouds (Kun, 1998)

Details Cepheus flare molecular clouds (Kun, 1998) Cepheus flare molecular clouds (Kun, 1998)

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..21150059k&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/115/59. Originally published in: 1998ApJS..115...59K

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Molecular Clouds, Ysos, Infrared Sources, Stars: Distances

Scientific paper

Results of an objective prism Schmidt survey are combined with IRAS survey data in order to assess the star-forming activity in the Cepheus Flare, a nearby giant molecular cloud complex at ~15{deg} above the Galactic equator. The distribution of absorbing matter along the line of sight was also studied. The Wolf diagrams, displaying the cumulative distribution of field star distance moduli, show that the interstellar matter in this region is concentrated at three characteristic distances: 200, 300, and 450pc. The three components, though partly overlapping, can be separated along the Galactic latitude. Within the area of the Cepheus Flare, distances are determined for 14 Lynds dark clouds and for some other clouds.
(4 data files).

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