Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/2573| Title: | Ultraviolet variability of HD 62001 - The central star of the missing nebula V-V 1-7 |
| Authors: | Kameswara Rao, N Gilra, D. P |
| Keywords: | Variable Stars Photometry Ultraviolet Spectroscopy |
| Issue Date: | Mar-1983 |
| Publisher: | Indian Academy of Sciences |
| Citation: | Journal of Astrophysics and Astronomy, Vol. 4, No. 1, pp. 59 – 63 |
| Abstract: | IUE observations of HD 62001 do not confirm the ultraviolet variability of 0.15 mag seen from the ANS observations. These intriguing variations in ANS observations seem to be caused by a nearby (∼ 70 arcsec away) B star getting in and out of the field of view of the telescope, which had a jitter of 20 arcsec. There seems to be no evidence for the presence of a hot companion, either from the energy distribution or from UV variability. However, visual light variations are present. This, coupled with the radial velocity variations, indicates a binary nature probably of Algol type. |
| Description: | Open Access |
| URI: | http://hdl.handle.net/2248/2573 |
| ISSN: | 0250-6335 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Ultraviolet variability | Open Access | 433.14 kB | Adobe PDF | ![]() View/Open |
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