IPs
AE Aqr
FO Aqr
XY Ari
V405 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
V709 Cas
V1025 Cen
TV Col
TX Col
UU Col
V2069 Cyg
V2306 Cyg
YY Dra
PQ Gem
DQ Her
EX Hya
NY Lup
V2400 Oph
GK Per
AO Psc
WX Pyx
V1223 Sgr
V1062 Tau
EI UMa
IGR 00234
IGR 15094
IGR 17303
Swift J0732
RX J0704
RX J1803
RX J2133
SDSS J233325
XSS 00564
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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).
- IP Credential:
- ***** (Ironclad)
- 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.
Tmax=HEJD 2452360.9113(1) + 0.00406634(2)E - (3.5+/-0.6)x10-14E2
(Mauche 2004)
- 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.
- Anzolin et al. 2010
- Anupama & Kantharia 1999
- Balman & Oegelman 1999
- Barlow et al. 2006
- Becker & Marshall 1981
- 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
- Brunschweiger et al. 2009
- Crampton, Cowley & Fisher 1986
- Cropper, Ramsay & Wu 1998a
- Eracleous, Patterson & Halpern 1991
- Eracleous, Halpern & Patterson 1991
- Evans & Hellier 2007
- Evans et al. 2009
- 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
- Landi et al. 2009
- Mattei 1996
- Mauche, Lee & Kallman 1997
- Mauche 2004
- 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
- Revnivtsev et al. 2008
- Richman 1996
- Rosino, Bianchini & Rafanelli 1982
- Sabbadi & Bianchini 1983
- Scaringi et al. 2010
- 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
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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