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Hubble COS Spectroscopy of the Dwarf Nova CW Mon: The White Dwarf in Quiescence?()
We present a synthetic spectral analysis of the HST COS spectrum of the U Geminorum-type dwarf nova CW Mon, taken during quiescence as part of our COS survey of accreting white dwarfs in Cataclysmic Variables. We use synthetic photosphere and optically thick accretion disk spectra to model the COS s...
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| Veröffentlicht in: | Astron J |
|---|---|
| Hauptverfasser: | , , , , , , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
2017
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| Schlagworte: | |
| Online Zugang: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5804891/ https://ncbi.nlm.nih.gov/pubmed/29430023 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/1538-3881/aa774c |
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