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The galatic and lmc extreme line supergiants compared: iue observations of the henize-carlson and zoo star samples of massive supergiants. [large magellanic cloud (lmc)]
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Sanduleak, N. Brown, D. N. Shore, S. N. Sonneborn, G. Bopp, B. W. Robinson, C. R. |
| Copyright Year | 1988 |
| Description | The Henize-Carlson sample of galactic massive supergiants, and a comparison between the Galactic and LMC samples are discussed. Several of the stars, notably He3-395 and S 127/LMC, have very similar shell characteristics. There appears to be little difference, other than luminosity, between the LMC and Galactic samples. One star, He3-1482, was detected with the Very Large Array at 6 cm. The UV data is combined with IRAS and optical information. |
| File Size | 324152 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19890001398 |
| Archival Resource Key | ark:/13960/t8gf5pz9w |
| Language | English |
| Publisher Date | 1988-06-01 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Stellar Spectra Magellanic Clouds Emission Spectra Spaceborne Astronomy Optical Properties Ultraviolet Spectra Iue Supergiant Stars Ultraviolet Astronomy Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |