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Discovery of two distorted interstellar bubbles
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Sofia, S. Gull, T. R. |
| Copyright Year | 1978 |
| Description | During an extensive program of direct imagery of emission nebulae, arcuate structures were found around two stars. A well-defined shock-like structure was found about the T-Orionis variable LL Orionis, located to the side of the Orion Nebula. A less extensive shock-like structure was also found about the runaway star zeta Ophiuchus. These structures can best be described in terms of distorted interstellar bubbles. A direct consequence of this interpretation is an independent estimate of the rates of mass loss for these stars. |
| File Size | 2560146 |
| Page Count | 20 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19790015682 |
| Archival Resource Key | ark:/13960/t4km43g2c |
| Language | English |
| Publisher Date | 1978-11-01 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Spectroscopy Bubbles Nebulae Interstellar Matter Stars Orion Constellation Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
