Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12323/5767Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Alimardanova, F. | - |
| dc.contributor.author | Miroshnichenko, A. S. | - |
| dc.contributor.author | Zharikov, S. V. | - |
| dc.contributor.author | Rudy, R. J. | - |
| dc.contributor.author | Manset, N. | - |
| dc.contributor.author | Kusakin, A. V. | - |
| dc.contributor.author | Kuratov, K. S. | - |
| dc.contributor.author | Khokhlov, S. | - |
| dc.date.accessioned | 2022-06-10T08:23:16Z | - |
| dc.date.available | 2022-06-10T08:23:16Z | - |
| dc.date.issued | 2017 | - |
| dc.identifier.citation | Astronomical Society of the Pacific | en_US |
| dc.identifier.uri | http://hdl.handle.net/20.500.12323/5767 | - |
| dc.description.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. | en_US |
| dc.language.iso | en | en_US |
| dc.relation.ispartofseries | Vol. 508; | - |
| dc.title | Spectroscopy and Photometry of MWC 137 | en_US |
| dc.type | Article | en_US |
| 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.