Hubble Space Telescope Imaging of the Outburst Site of M31 RV. II. No Blue Remnant in Quiescence
Howard E. Bond (Space Telescope Science Institute)

TL;DR
This study re-examines HST data of M31 RV's 1988 outburst site, debunking previous claims of a hot remnant and concluding no detectable blue remnant exists in the observed field.
Contribution
The paper provides a detailed re-analysis of archival HST images, correcting prior misinterpretations and clarifying the nature of the remnant of M31 RV after its outburst.
Findings
No evidence of a hot, blue remnant in the HST images.
Previous UV and hot star detections were due to cosmic rays and misinterpretation.
M31 RV's remnant is either undetectable, a red giant companion, or an unresolved red giant.
Abstract
M31 RV is a red transient that erupted in 1988 in the Andromeda bulge, reaching a luminosity intermediate between novae and supernovae. It was cool throughout its outburst, unlike a normal classical nova. In 2006, Bond & Siegel examined archival HST optical images of the M31 RV site, obtained in 1999. We found only old red giants at the site, and no stars of unusual color. However, Shara et al. recently claimed to have detected (a) a bright UV source within the error box in HST UV images taken in 1995, (b) a hot (Teff>40,000 K) optical source in the same 1999 images that we examined, and (c) cooling of this source from 1999 to 2008. Shara et al. argue that this source's behavior is consistent with a classical-nova outburst occurring on a low-mass white dwarf. I have re-examined all of the HST frames, including new ones obtained in 2009-2010. I find that: (a) the bright 1995 UV…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
