Darnley, MJ and Starrfield, S (2018) On the progenitor system of V392 Persei. Research Notes of the American Astronomical Association RN AAS, 2 (2). ISSN 2515-5172

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Abstract

A discussion regarding the progenitor system of the nova and dwarf nova system V392 Persei using archival data from 2MASS and WISE. We find that the system is unlikely to contain a luminous red giant donor (i.e. a symbiotic system), but cannot exclude the presence of a lower luminosity red giant or a sub-giant donor. The similarity of the SED of the quiescent V392 Per to that of GK Persei is noted.

Item Type:	Article
Uncontrolled Keywords:	astro-ph.SR; astro-ph.SR; astro-ph.HE
Subjects:	Q Science > QB Astronomy Q Science > QC Physics
Divisions:	Astrophysics Research Institute
Publisher:	American Astronomical Society; IOP Publishing
Related URLs:	http://arxiv.org/abs/1805.00994v1
Date Deposited:	08 May 2018 09:33
Last Modified:	04 Sep 2021 02:42
DOI or ID number:	10.3847/2515-5172/aac26c
URI:	https://researchonline.ljmu.ac.uk/id/eprint/8627

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