Confirmation of the planetary nebula nature of HaTr 5. Not the remnant of Nova Sco 1437

The identification of the nebula HaTr 5 with the shell remnant of the historic Nova Sco 1437 around the low-accretion rate cataclysmic variable 2MASS J17022815-4306123 has been used in the framework of the hibernation scenario to set an upper limit of

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Bibliographische Detailangaben
Hauptverfasser:	Guerrero, M. A, Santamaria, E, Liberato, G, Parker, Q. A, Goncalves, D. R, Rodriguez-Gonzalez, J. B, Ritter, A, Yuan, H, Toala, J. A
Format:	Artikel
Sprache:	eng
Schlagworte:	Physics - Astrophysics of Galaxies Physics - Solar and Stellar Astrophysics
Online-Zugang:	Volltext bestellen
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Beschreibung
Zusammenfassung:	The identification of the nebula HaTr 5 with the shell remnant of the historic Nova Sco 1437 around the low-accretion rate cataclysmic variable 2MASS J17022815-4306123 has been used in the framework of the hibernation scenario to set an upper limit of
DOI:	10.48550/arxiv.2412.12813