[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-campaign-nova 173] Re: (fwd) V445 Pup (Eyres)
Re: (fwd) V445 Pup (Eyres)
> > A number of symbiotic stars, particularly the so-called symbiotic
> > novae (e.g. HM Sge) have spectra early in their outbursts which show
> > no hint of a red giants, and often these objects were not even
> > identified as symbiotic stars until outburst. Also, as far as I can
> > tell some symbiotic novae (e.g. HM Sge, V1016 Cyg) do not appear in
> > the 2MASS Second Incremental Release Point Source Catalog. The
> > H-deficiency is harder to explain in the symbiotic model however.
>
> They are very bright 2MASS sources.
Furthermore, these two stars show Mira-type pulsations in the JHK bands,
which shows the M-type star is clearly visible in the near-IR.
Regards,
Taichi Kato
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp