GK Persei = Nova Persei 1901
SkyView image
of GK Per (see important notes).
- Position:
-
- Equatorial: 03h31m12.0s,
+43d54m17s (J2000)
- Galactic: l=150.96, b=-10.10
- Finding Chart:
- williams?
- Brightness:
- Optical: mv~13.5 in quiescence, ~10.5 during minor outbursts;
fx (2-10 keV)~3.2x10-11 ergs/cm/cm/s in quiescence (ASCA),
1.9x10-10 ergs/cm/cm/s in outburst (ASCA).
- Periods:
-
- Orbital: 1.996803 d = 47.923272 hr = 172523.78 s,
seen in optical spectroscopy.
Secondary's maximum redshift at HJD2444912.966(8)+1.996803(7)E
(Crampton et al 1986)
- Spin: 0.0040625 d = 5.85 min = 351s, seen in X-rays and optical.
Ephemeris?
- Others: ?
- Inclination:
- 46 < i < 73
- Distance:
- 470 pc (nova shell)
GK Per is a giant among Intermediate Polars, with a highly developed disk.
References
We will not even attempt to list pre-1980 papers
that deal exclusively with the classical nova event of 1901; see the
Bode and Evans book on Classical Novae for that.
- Anupama & Kantharia 1999
- Balman & Oegelman 1999
- Bianchini & Sabbadin 1983
- Bianchini & Sabbadin 1985
- Bianchini, Sabbadin & Hamzaoglu 1981
- Bianchini, Sabbadin & Hamzaoglu 1982
- Bianchini et al 1986
- Bianchini et al 2003
- Bode et al 1987
- Crampton, Cowley & Fisher 1986
- Cropper, Ramsay & Wu 1998a
- Eracleous, Patterson & Halpern 1991
- Eracleous, Halpern & Patterson 1991
- Ezuka & Ishida 1999
- Garlick et al 1994b
- Hellier 1992
- Hellier & Livio 1994
- Hellier & Mukai 2004
- Hellier, Mukai & Osborne 1998a
- Hellier, Harmer & Beardmore 2004
- Hessman et al 1989
- Hutchings & Cote 1986
- Ishida 1991
- Ishida et al 1992
- King, Ricketts & Warwick 1979
- Kraft 1964
- Mattei 1996
- Mauche, Lee & Kallman 1997
- Mazeh et al 1985
- Morales-Rueda, Still & Roche 1999
- Morales-Rueda et al 2002
- Mukai et al 2003
- Mumford 1968
- Nogami, Kato & Baba 2002
- Norton, Watson & King 1988
- Norton & Watson 1989b
- Patterson 1981
- Patterson 1991
- Pezzuto, Bianchini & Stagni 1996
- Reinsch 1994
- Richman 1996
- Rosino, Bianchini & Rafanelli 1982
- Sabbadi & Bianchini 1983
- Seaquist et al 1989
- Simon 2002
- Stockman et al 1992
- Suleimanov, Revnivtsev & Ritter 2005
- Szkody, Mateo & Mattei 1985
- Vrielmann, Ness & Schmitt 2005
- Watson, King & Osborne 1985
- Wu et al 1989