IPs
V455 And
V515 And
AE Aqr
FO Aqr
V349 Aqr
XY Ari
V405 Aur
V647 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
V709 Cas
V1025 Cen
V1033 Cas
TV Col
TX Col
UU Col
V2069 Cyg
V2306 Cyg
DO Dra
PQ Gem
V418 Gem
DQ Her
V1323 Her
V1460 Her
V1674 Her
EX Hya
NY Lup
V2400 Oph
V2731 Oph
V3037 Oph
V598 Peg
GK Per
AO Psc
HZ Pup
V667 Pup
WX Pyx
V1223 Sgr
V4743 Sgr
CC Scl
V1062 Tau
EI UMa
AX J1740.1
AX J1832.3
AX J1853.3
CTCV J2056
CXO J174954
IGR J04571
IGR J08390
IGR J15094
IGR J16500
IGR J16547
IGR J17014
IGR J17195
IGR J18151
IGR J18173
IGR J18308
IGR J19267
LAMOST 0240
PBC J0927.8
PBC J1841.1
RX J1804
RX J2015
RX J2113
RX J2133
RX J2306
Swift J0717
Swift J1839
Swift J2006
Swift J2138
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TV Columbae = A0526-328
Links to this object in
VSX
and in
Swift BAT 157 month survey
SkyView image
of TV Col (see important notes);
the IP is the SE component of the close pair.
- Position:
-
- Equatorial: 05h29m25.54s,
-32d49m03.5s (Gaia)
- Galactic: l=236.79, b=-30.60
- Finding Chart:
- Charles et al. (1979)
- Brightness:
- Optical: G=14.0 (Gaia); X-rays: 5.9x10-11 ergs cm-2s-1 (BAT 157m; 14-195 keV), 6.0x10-11 ergs cm-2s-1 (2SXPS)
- IP Credential:
- ***** (Ironclad) The spin period has been repeatedly detected in multiple
X-ray observations, although it remains elusive in optical photometry. The
orbital period is from optical photometry and from the grazing eclipse.
- Periods:
-
- Orbital: 0.2285999 d = 5.486398 hr = 19751.03 s, from partial eclipes
in the optical
HJD(eclipse) = 2448267.4893(5) + 0.2285999(2)E
(Hellier (1993))
- Spin: 0.0221 d = 31.83 min = 1909.7(2.5) s, seen in X-rays.
- Others: 5.2 hr photometric period and 4-day beat between orbit and 5.2hr.
- Inclination:
- ~70 (has grazing eclipse).
- Distance:
- 502.8 (499.3-506.9) pc (Gaia EDR3; parallax: 1.951+/-0.014 mas)
References
- Charles et al. 1979 (optical spectroscopy)
- Schwartz et al. 1979 (optical identification of X-ray sources)
- Warner 1980 (optical photometry)
- Watts, Greenhill & Thomas 1980 (optical spectroscopy)
- Coe & Wickramasinghe 1981 (ultraviolet)
- Motch 1981 (optical photometry)
- Patterson 1981 (X-ray to optical flux ratios)
- Mouchet et al. 1981 (ultraviolet)
- Hutchings et al. 1981 (optical spectroscopy)
- Watts et al. 1982 (X-rays, optical spectroscopy & photometry)
- Szkody & Mateo 1984 (UV and optical during outburst)
- Mateo, Szkody & Hutchings 1985 (ultraviolet spectroscopy)
- Watts 1985 (beating of photometric modulations)
- Bonnet-Bidaud, Motch & Mouchet 1985 (ultraviolet to infrared photometry)
- Penning, Schmidt & Liebert 1986 (optical polarimetry)
- Warner 1986 (optical sidebands)
- Schrijver, Brinkman & van der Woerd 1987 (X-rays)
- Bookbinder & Lamb 1987 (radio)
- Schwarz et al. 1988 (optical spectroscopy & photometry during outburst)
- Barrett, O'Donoghue & Warner 1988 (optical photometry)
- Norton & Watson 1989a (spin equilibrium)
- Norton & Watson 1989b (X-rays)
- Angelini & Verbunt 1989 (outburst)
- Hellier, Mason & Mittaz 1991a (optical photometry)
- Eracleous, Patterson & Halpern 1991 (X-ray timing)
- Ishida 1991 (X-rays)
- Hellier 1991 (disk or not?)
- Eracleous, Halpern & Patterson 1991 (X-ray spectroscopy)
- Hellier 1992 (X-ray timing)
- Stockman et al. 1992 (optical polarimetry)
- Hellier, Garlick & Mason 1993 (X-rays - orbital modulation)
- Hellier 1993 (optical photometry & spectroscopy)
- Hellier & Buckley 1993 (optical photometry & spectroscopy during outburst)
- Augusteijn et al. 1994 (optical photometry)
- Vrtilek et al. 1996 (X-ray spectroscopy)
- Mauche, Lee & Kallman 1997 (ultraviolet spectroscopy)
- Cropper, Ramsay & Wu 1998 (X-ray spectroscopy)
- Hellier, Mukai & Osborne 1998 (X-ray spectroscopy)
- Ezuka & Ishida 1999 (X-ray spectroscopy)
- Cropper et al. 1999 (post-chock model with gravity)
- Ramsay 2000 (X-ray spectroscopy)
- McArthur et al. 2001 (parallax)
- Retter et al. 2003 (optical photometry)
- Rana et al. 2004 (X-ray timing)
- Suleimanov, Revnivtsev & Ritter 2005 (X-ray spectroscopy)
- Parker, Norton & Mukai 2005 (X-ray timing)
- Brunschweiger et al. 2009 (X-rays)
- Scaringi et al. 2010 (X-rays)
- Yuasa et al. 2010 (X-ray spectroscopy)
- Dai et al. 2010 (optical photometry)
- Galis et al. 2010 (X-rays)
- Revnivtsev et al. 2011 (X-ray and optical photometry)
- Pretorius, Kingge & Schwope 2013 (space density)
- Pretorius & Mukai 2014 (space density)
- Hailey et al. 2016 (X-rays)
- Hameury & Lasota 2017 (disk instability model for IPs)
- Barrett et al. 2017 (radio)
- Sanad & Abdel-Sabour 2018 (ultraviolet)
- Campana et al. 2018 (optical & multiwavelength)
- Schwope 2018 (space density)
- Suleimanov, Doroshenko & Werner 2019 (X-ray spectroscopy)
- Lopes de Oliveira & Mukai 2019 (X-rays)
- Simon 2021 (optical photometry)
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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