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The appearance of the gum nebula
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Bok, B. J. |
| Copyright Year | 1971 |
| Description | The dimensions of the Gum nebula complex appear to be overestimated. The distance of 460 parsecs to the central pulsar is rather on the large side, and likely contributions from gamma Velorum and zeta Puppis were underestimated. The multiorigin character of the Gum nebula is reaffirmed. The parts produced by traditional ultraviolet thermal radiation and by processes directly related to the supernova outburst must be defined. |
| File Size | 1219743 |
| Page Count | 5 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19720004118 |
| Archival Resource Key | ark:/13960/t48q0s26x |
| Language | English |
| Publisher Date | 1971-09-01 |
| Access Restriction | Open |
| Subject Keyword | Space Sciences Origins Ultraviolet Radiation Thermal Radiation Hot Stars Conferences Supernovae Pulsars Size Dimensions Nebulae Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
