SAO 75669: A late type giant behind the molecular cloud MBM 12

Details SAO 75669: A late type giant behind the molecular cloud MBM 12 SAO 75669: A late type giant behind the molecular cloud MBM 12

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...289..946b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 289, no. 3, p. 946-948

Astronomy and Astrophysics

Astrophysics

2

Giant Stars, Infrared Spectra, Interstellar Extinction, Interstellar Matter, M Stars, Molecular Clouds, Stellar Magnitude, Visible Spectrum, Absorptance, Astronomical Polarimetry, Flux Density, Spectrum Analysis, Stellar Spectrophotometry

Scientific paper

Photometric and spectroscopic observations of the star SAO 75669 in the region of the high galactic latitude molecular cloud MBM 12 are presented. The optical, near-infrared and far-infrared IRAS photometric magnitudes together with the observed CCD spectrum and the large degree of polarization are consistent with the star being and M type giant behind the molecular cloud MBM 12 suffering about 1.8 magnitudes visual extinction. The wavelength dependence of polarization indicates that the dust in the cloud is normal.

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