Carbon star reddenings and low latitude H I column densities

Details Carbon star reddenings and low latitude H I column densities Carbon star reddenings and low latitude H I column densities

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....101.1756s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 101, May 1991, p. 1756-1762.

Astronomy and Astrophysics

Astronomy

4

Carbon Stars, Interstellar Extinction, Astronomical Photometry, Cosmic Dust, Stellar Color

Scientific paper

Foreground H I column densities are computed toward 564 low latitude northern and southern hemisphere carbon stars, using photometric distances and an assumed rotation curve. Separate dust-to-H I ratios and dereddened (J-H, H-K) loci are obtained for the two hemispheres. A small but statistically significant difference is found between the two samples, which is attributed to a small difference in photometric systems.

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