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- W3019491749 abstract "Nova LMC 1995 was detected with ROSAT as an X-ray source in repeated observations between 1995 and 1998, starting five months after the outburst. In February 1998, 3 years after the nova outburst, ROSAT PSPC data show that this is the only LMC post-nova - and one out of three among '100 altogether - that appeared as a bright supersoft X-ray source after the outburst. The PSPC data are satisfactorily fitted with an LTE carbon-oxygen atmosphere model for a 1.2 M white dwarf, resulting in an effective temperature about 30 eV. The X-ray flux increased in the last years and at present Nova LMC 1995 is about twice as bright as in a 1996 observation. We suggest that the photosphere is still shrinking and the remnant becoming hotter. Such a nova is a likely type Ia SN progenitor." @default.
- W3019491749 created "2020-05-01" @default.
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- W3019491749 date "1998-12-01" @default.
- W3019491749 modified "2023-09-27" @default.
- W3019491749 title "LMC 1995, the third Supersoft X-ray Nova" @default.
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- W3019491749 hasPublicationYear "1998" @default.
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