Bhatt, H. C. ; Sagar, R. ; Subramaniam, A. ; Gorti, U. ; Chandrasekhar, T. ; Ashok, N. M. ; Ragland, S. (1994) SAO 75669: A late type giant behind the molecular cloud MBM 12 Astronomy & Astrophysics, 289 (3). pp. 946-948. ISSN 0004-6361
![[img]](https://repository.ias.ac.in/style/images/fileicons/application_pdf.png)
|
PDF
- Publisher Version
67kB |
Official URL: http://adsabs.harvard.edu/abs/1994A%26A...289..946...
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.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to EDP Sciences. |
| Keywords: | SAO 75669; Interstellar Medium; Molecular Clouds |
| ID Code: | 67773 |
| Deposited On: | 31 Oct 2011 13:33 |
| Last Modified: | 18 May 2016 14:44 |
Repository Staff Only: item control page
