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

Bhatt, H. C; Sagar, R; Subramaniam, A; Gorti, U; Chandrasekhar, T; Ashok, N. M; Ragland, S

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dc.contributor.author	Bhatt, H. C
dc.contributor.author	Sagar, R
dc.contributor.author	Subramaniam, A
dc.contributor.author	Gorti, U
dc.contributor.author	Chandrasekhar, T
dc.contributor.author	Ashok, N. M
dc.contributor.author	Ragland, S
dc.date.accessioned	2008-07-14T06:10:50Z
dc.date.available	2008-07-14T06:10:50Z
dc.date.issued	1994-09
dc.identifier.citation	Astronomy and Astrophysics, Vol. 289, No. 3, pp. 946 - 948	en
dc.identifier.issn	0004-6361
dc.identifier.uri	http://hdl.handle.net/2248/2659
dc.description.abstract	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.	en
dc.format.extent	378100 bytes
dc.format.mimetype	application/pdf
dc.language.iso		en
dc.publisher	European Southern Observatory	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1994A%26A...289..946B	en
dc.subject	Giant stars	en
dc.subject	Infrared Spectra	en
dc.subject	Interstellar Extinction	en
dc.subject	Interstellar Matter	en
dc.subject	M Stars	en
dc.subject	Molecular Clouds	en
dc.subject	Stellar Magnitude	en
dc.subject	Visible Spectrum	en
dc.subject	Absorptance	en
dc.subject	Astronomical Polarimetry	en
dc.subject	Flux Density	en
dc.subject	Spectrum Analysis	en
dc.subject	Stellar Spectrophotometry	en
dc.title	SAO 75669: A late type giant behind the molecular cloud MBM 12	en