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Coordinated observations of interacting peculiar red giant binaries, 1
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Ake, T. |
| Copyright Year | 1995 |
| Description | IUE Observations were begun for a two-year program to monitor the UV variability of three interacting peculiar red giant (PRG) binaries, HD 59643 (C6,s) HD 35155 (S3/2), and HR 1105 (S3.5/2.5). All of these systems were suspected to involve accretion of material from the PRG to a white-dwarf secondary, based mainly on previous IUE investigations. From our earlier surveys of PRG's, they were primary candidates to test the hypothesis that Tc-poor PRG's are formed as a result of mass transfer from a secondary component rather than from internal thermal pulsing while on the asymptotic red giant branch. |
| File Size | 1134178 |
| Page Count | 13 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19960012169 |
| Archival Resource Key | ark:/13960/t6vx5912j |
| Language | English |
| Publisher Date | 1995-12-01 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Red Giant Stars Time Series Analysis Ultraviolet Spectra H Alpha Line Periodic Variations Asymptotic Giant Branch Stars Mass Transfer Stellar Mass Accretion Hypotheses Binary Stars Iue Companion 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 | Technical Report |