The distance and structure of L379

Details The distance and structure of L379 The distance and structure of L379

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....106..672h&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 106, no. 2, p. 672-675, 825.

Astronomy and Astrophysics

Astronomy

4

Plasma Clouds, Star Formation, Stellar Spectrophotometry, Ubv Spectra, F Stars, Faint Objects, G Stars

Scientific paper

UBV and H-beta photometry has been carried out on 107 stars located within the more obscured region of the dark galactic cloud L379. Most of the measured stars are fainter than 10.0 m and their spectral classification is not available in the literature. Spectral types were found for 47 stars using movement along the reddening line coupled with the assumption that all stars are on the main sequence. For each star, the extinction A(v) (mag) and the distance r(kpc) were derived, and from the A(v)-r graph, an attempt was made to determine the structure of L379.

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