Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2659
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dc.contributor.authorBhatt, H. C-
dc.contributor.authorSagar, R-
dc.contributor.authorSubramaniam, A-
dc.contributor.authorGorti, U-
dc.contributor.authorChandrasekhar, T-
dc.contributor.authorAshok, N. M-
dc.contributor.authorRagland, S-
dc.date.accessioned2008-07-14T06:10:50Z-
dc.date.available2008-07-14T06:10:50Z-
dc.date.issued1994-09-
dc.identifier.citationAstronomy and Astrophysics, Vol. 289, No. 3, pp. 946 - 948en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/2659-
dc.description.abstractPhotometric 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.extent378100 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1994A%26A...289..946Ben
dc.subjectGiant starsen
dc.subjectInfrared Spectraen
dc.subjectInterstellar Extinctionen
dc.subjectInterstellar Matteren
dc.subjectM Starsen
dc.subjectMolecular Cloudsen
dc.subjectStellar Magnitudeen
dc.subjectVisible Spectrumen
dc.subjectAbsorptanceen
dc.subjectAstronomical Polarimetryen
dc.subjectFlux Densityen
dc.subjectSpectrum Analysisen
dc.subjectStellar Spectrophotometryen
dc.titleSAO 75669: A late type giant behind the molecular cloud MBM 12en
Appears in Collections:IIAP Publications

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