Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12323/5767| Title: | Spectroscopy and Photometry of MWC 137 |
| Authors: | Alimardanova, F. Miroshnichenko, A. S. Zharikov, S. V. Rudy, R. J. Manset, N. Kusakin, A. V. Kuratov, K. S. Khokhlov, S. |
| Issue Date: | 2017 |
| Citation: | Astronomical Society of the Pacific |
| Series/Report no.: | Vol. 508; |
| Abstract: | MWC 137 is an object with a strong emission-line spectrum associated with an 1'-size H Imall> region Sharpless 266. It was included in a catalog of planetary nebulae in 1967, in the first list of objects with the B[e] phenomenon in 1976, and in a list of Herbig Ae/Be stars in 1984. A recent analysis of the stellar and nebular spectra of MWC 137 by several authors suggested that it is most likely a B[e] supergiant located at a distance 4-6 kpc away from the Sun. No high-resolution spectra of the object have been published so far. We present the results of our analysis of high-resolution optical spectra of MWC 137 obtained in 2004-2016 and UBVRI photometry. |
| URI: | http://hdl.handle.net/20.500.12323/5767 |
| Appears in Collections: | Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Spectroscopy and Photometry of MWC 137.pdf | 40.01 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.