Other Names	2U 0114+63, 3U 0115+63, 4U 0115+635, V* V635 Cas, X0115+63
INTEGRAL source ID	J011831.9+634424
External database entries	Simbad, ADS, ISDC
Discovery	Giacconi et al. (1972)
Dominant Accretion Type	Transient X-ray source, Be binary, HMXB
Position RA, DEC	01h 18m 31.9s  19.632917deg	+63d 44m 24s  +63.740000deg	Johnston et al. (1978)
Position l,b	125.92	+1.03
Distance	8(1) kpc		Negueruela et al. (2001a)
Typical Flux	0.4 Crab	Energy Range	1 - 20 keV

Neutron Star Mass	+ -
Neutron Star Luminosity

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The given typical flux is the maximum flux in a strong outburst. Outbursts, e.g., in 1969/70 (3x), 1971, 1974, 1977/78, 1980 (2x), 1985, 1987, 1990, 1994, 1999, 2000. See, e.g.: Forman, Tananbaum & Jones (1976) Whitlock et al. (1989) Tamura et al. (1992) Bildsten et al. (1997) Negueruela et al. (1997) Heindl et al. (1999) Maybe there is an approximately 3 year recurrence time scale for strong bursts and an additional 6-9 months time scale (Whitlock et al., 1989; Negueruela et al., 2001b).

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Last modification date: Fri Aug 3 01:06:13 2007