pith. sign in

arxiv: 1810.10131 · v1 · pith:4KP2YA52new · submitted 2018-10-23 · 🌌 astro-ph.SR

Photometric Observations of the 2017 Outburst of Recurrent Nova M31N 2007-10b

Quentin J. Socia , Martin Henze , Allen W. Shafter , J. Chuck Horst This is my paper
classification 🌌 astro-ph.SR
keywords m31nrecurrentnovaobservationsoutburstphotometricrecurrenceat2017jdm
0
0 comments X
read the original abstract

M31 is an ideal laboratory for observing and studying recurrent novae. To date, there have been 18 recurrent nova discovered in M31, six of which have recurrence periods less than nine years. M31N 2017-12a (AT2017jdm) is a transient that was reported near the center of M31, with the time of outburst estimated to be 2017 December 24.141 +/- 0.42 based on constraints from previous data. Here we present the photometric observations of M31N 2017-12a, which we confirm as a recurrence of M31N 2007-10b.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The Recurrent Nova Population in M31

    astro-ph.SR 2026-04 accept novelty 4.0

    M31 hosts at least 20 recurrent novae with 79 total eruptions; half recur faster than the shortest Galactic example, while light-curve and spatial properties match the Milky Way population.