A&A 396, 629-632 (2002)
DOI: 10.1051/0004-6361:20021519
Research Note
Is KT Mon a classical nova?
T. Kato1 and H. Yamaoka21 Department of Astronomy, Kyoto University, Kyoto 606-8502, Japan
2 Faculty of Science, Kyushu University, Fukuoka 810-8560, Japan
(Received 23 September 2002 / Accepted 15 October 2002 )
Abstract
KT Mon has been considered as a classical nova in 1942 based on its
light curve and spectroscopy. However, we noticed a unusual feature
for a nova soon after its maximum: the early presence of high excitation
emission lines such as HeII and NIII.
We propose previously overlooked interpretations that KT Mon can be either
a WZ Sge-type dwarf nova and an X-ray transient, although the possibility
of an unusual or a recurrent nova is not completely excluded.
If KT Mon is a WZ Sge-type dwarf nova, the system is expected to have
a brown dwarf secondary.
If KT Mon is an X-ray transient, the system is a good candidate for the
nearest black-hole binary. Within our knowledge, the observed features
seem to more strongly support the latter possibility.
In all possibilities, we can expect a recurrent outburst in meaningfully
near future.
Key words: accretion, accretion disks -- novae, cataclysmic variables -- stars: dwarf novae -- X-rays: bursts -- stars: individual: KT Mon
Offprint request: T. Kato, tkato@kusastro.kyoto-u.ac.jp
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