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On the progenitor system of V392 Persei

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

1805.00994v1.pdf - Accepted Version

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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:
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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