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V597 Puppis = Nova Puppis 2007

Link to this object in VSX

A finding chart for V597 Pup

SkyView image of V597 Pup (see important notes)

Position
Finding Chart:
Warner & Woudt (2009)
Brigntness:
Optical G=20.0 (Gaia); X-rays: 9.3x10-15 ergs cm-2s-1 (4XMM-DR11)
IP Credential:
** (Possible): While the orbital period is beyond doubt, the 524 s signal was originally detected when accretion component couldn't have been the dominant light source (an eclipse was not obvious then), and weakened as the post-nova became fainter and a deep eclipse revealed itself. This is strange for a spin signal of an IP.
Periods:
Inclination:
High (eclipsing)
Distance:
>1.65 kpc (DR2 parallax uncertain)
4800 (2900-6800) pc (Gaia EDR3; parallax: 0.303+/-0.395 mas)

References

  1. Warner & Woudt 2003 (optical photometry)
  2. Naik, Banerjee & Ashok 2009 (infrered spectroscopy)
  3. Worpel et al. 2020 (X-rays)


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