Obscuration effects in super-soft-source X-ray spectra

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Volume 559 (November 2013)

A&A, 559 (2013) A50

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Table 1

Description of targets.

Target Type/sub-type^at_ref^b			i^c	d^d

Persistent SSS
Cal 83	SSS/SSa	–	20−30^1,2	48.1 ± 2.9³
Cal 87	SSS/SSe	–	73−77^4,5	48.1 ± 2.9³
RX J0513.9-6951	SSS/SSa	–	~35⁶	48.1 ± 2.9³
QR And^e	SSS/SSe	–35−60⁷; > 79^8,9,10		2.0¹⁰
Classical Novae (CNe)
HV Cet^f	CN/SSe	2008-10-07.4	high¹¹?	4.5 ± 2.0¹²
LMC 2012	CN/SSa	2012-03-26.4	?	48.1 ± 2.9³
V959 Mon	CN/SSe	2012-08-09.8	82 ± 6¹⁶	1.5¹⁷
V1494 Aql	CN/SSe	1999-12-01.8	78.5^18,19,20	1.6 ± 0.1²¹
V5116 Sgr	CN/SSa,e	2005-07-04.0	high^24,26	11 ± 3²⁵
V723 Cas	CN/SSa	1995-08-24.0	62^26,27	3.9 ± 0.2²⁶
V382 Vel	CN/neb	1999-05-22.4	25−67²⁸	1.7 ± 0.3²⁹
V4743 Sgr	CN/SSa	2002-09-19.8	?	3.9 ± 0.3¹⁵
KT Eri^g	CN/SSa	2009-11-14.6	58¹³	6.5¹⁴
V2491 Cyg^g	CN/SSa	2008-04-10.7	80²²?	10.5²³
LMC 2009a^g	RN/SSe	2009-02-05.1	?	48.1 ± 2.9³
Recurrent Novae (RNe) ^b
RS Oph	RN/SSa	2006-02-12.8	30−40^30,31	1.6 ± 0.3^32,33
U Sco	RN/SSe	2010-01-27.8	82^34,35	12 ± 2³⁶
T Pyx	RN/neb	2011-04-14.3	< 20^37,38,39	4.8 ± 0.5^37,40

Notes.

^(a)

CN: Classical Nova; RN: Recurrent Nova; SSS: persistent Super Soft Source. Sub-types are given indicating absorption-line dominated X-ray spectra (SSa: Sect. 3.2), emission line dominated spectra (SSe: Sect. 3.3), and post-outburst nebular spectra (neb: Sect. 3.6). The clearest cases are given in bold face while intermediate or less clear cases are given in italic. V5116 Sgr transitions between SSa and SSe, marked by SSa,e (Sect. 3.5).

^(b)

Discovery date for CNe and RNe used as reference time (latest outburst for RNe).

^(c)

Inclination angle in degrees.

^(d)

Distance (kpc); for LMC novae, the distance to the LMC is given.

^(e)

Aka RX J0019.8+2156.

^(f)

Aka CSS081007:030559+054715.

^(g)

Possible RN.

Reference.

⁽¹⁾

Crampton et al. (1987);

⁽²⁾

Schmidtke & Cowley (2006);

⁽³⁾

Macri et al. (2006);

⁽⁴⁾

Schandl et al. (1997);

⁽⁵⁾

Ebisawa et al. (2001);

⁽⁶⁾

Hutchings et al. (2002);

⁽⁷⁾

Becker et al. (1998) (35 < i < 60);

⁽⁸⁾

Kahabka (1996);

⁽⁹⁾

Tomov et al. (1998) (i > 79);

⁽¹⁰⁾

Beuermann et al. (1995);

⁽¹¹⁾

Beardmore et al. (2012);

⁽¹²⁾

Schwarz et al. (2008);

⁽¹³⁾

Ribeiro et al. (2013a);

⁽¹⁴⁾

Ragan et al. (2009);

⁽¹⁵⁾

Vanlandingham et al. (2007);

⁽¹⁶⁾

Ribeiro et al. (2013b);

⁽¹⁷⁾

Munari et al. (2013);

⁽¹⁸⁾

Bos et al. (2001);

⁽¹⁹⁾

Barsukova & Goranskii (2003);

⁽²⁰⁾

Hachisu et al. (2004);

⁽²¹⁾

Iijima & Esenoglu (2003);

⁽²²⁾

Ribeiro et al. (2011);

⁽²³⁾

Helton et al. (2008);

⁽²⁴⁾

Dobrotka et al. (2008);

⁽²⁵⁾

Sala et al. (2008);

⁽²⁶⁾

Lyke & Campbell (2009);

⁽²⁷⁾

Goranskij et al. (2007);

⁽²⁸⁾

Shore et al. (2003);

⁽²⁹⁾

Della Valle et al. (2002);

⁽³⁰⁾

Dobrzycka & Kenyon (1994);

⁽³¹⁾

Ribeiro et al. (2009);

⁽³²⁾

Bode (1987);

⁽³³⁾

Barry et al. (2008);

⁽³⁴⁾

Schaefer (1990);

⁽³⁵⁾

Thoroughgood et al. (2001);

⁽³⁶⁾

Schaefer (2010);

⁽³⁷⁾

Chesneau et al. (2011);

⁽³⁸⁾

Uthas et al. (2010);

⁽³⁹⁾

Sokoloski et al. (2013);

⁽⁴⁰⁾

Shore et al. (2011).

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