Issue |
A&A
Volume 541, May 2012
|
|
---|---|---|
Article Number | A98 | |
Number of page(s) | 10 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201118389 | |
Published online | 10 May 2012 |
Online material
The main parameters of the interacting planetary nebulae sample.
Notes. References for interaction: (1) Soker (1997); (2) Wareing et al. (2007); (3) Rauch & Kerber (2005); (4) Borkowski et al. (1990); (5) Tweedy & Kwitter (1996); (6) Dgani & Soker (1998); (7) Soker (1999); (8) Ramos-Larios et al. (2011); (9) Tweedy & Kwitter (1994a); (10) Rauch et al. (2004); (11) Jacoby (1981); (12) Kwitter et al. (1988); (13) Xilouris et al. (1996); (14) Pierce et al. (2004); (15) Kerber et al. (1997); (16) Kerber et al. (2000a); (17) Kerber (1998); (18) Ali & Pfleiderer (1999); (19) Soker & Hadar (2002); Zucker & Soker (1993); (21) Jacoby & Van de Steene (1995); (22) Frew et al. (2011); (23) Kerber et al. (1998); (24) Ali et al. (2000); (25) Rauch et al. (2000); (26) Bond & Livio (1990); (27) Corradi et al. (2003); (28) Guerrero et al. (1998); (29) Martin et al. (2002); (30) Villaver et al. (2003); (31) Kerber et al. (2000b); (32) Ramos-Larios & Phillips (2009); (33) Wareing (2010); (34) Muthu et al. (2000); (35) Rauch (1999); (36) Corradi & Schwarz (1995); (37) Weinberger & Aryal (2004); (38) Aryal et al. (2009); (39) Guerrero et al. (2003); (40) Borkowski (1993); (41) Clark et al. (2010); (42) Chu et al. (1991); (43) Soker & Zucker (1997); (44) Tweedy & Kwitter (1994b); (45) Tweedy & Napiwotzki (1994); (46) Tweedy et al. (1995).
References for IPNe distance: (1) Pottasch (1996); (2) Harris et al. (2007); (3) Pottasch & Acker (1998); (4) Acker et al. (1998); (5) Zhang (1993); (6) Sabbadin (1986); (7) Pottasch (1983); (8) Cazetta & Maciel (2001); Kaler & Feibelman (1985); (10) Kaler et al. (1985); (11) Napiwotzki (2001); (12) Napiwotzki (1999); (13) Saurer (1995); (14) Benedict et al. (2009); (15) Rauch et al. (1996); (16) Giammanco et al. (2011); (17) Cahn & Kaler (1971); (18) Ali & Basurah (2008); (19) Napiwotzki & Schonberner (1995); (20) Ali (2006); (21) Bensby & Lundstrom (2001); (22) Mellema (2004); (23) Gathier et al. (1986); (24) Jacoby et al. (1997); (25) Kerber et al. (1998); (26) Hartl & Weinberger (1987); (27) Tajitsu & Tamura (1998); (28) Weinberger & Sabbadin (1981); (29) Werner et al. (1991); (30) Dengel et al. (1980); (31) Cudworth & Peterson (1988); (32) Cudworth (1990); (33) Frew et al. (2010); (34) Rauch et al. (2004).
∗“Ind.” means individual distance, “Ph02” means distances calculated according to Phillips distance scale (2002) and “St.” means statistical distances from literature.
References for IPNe radius: (1) ESO-Strasburg Catalog; (2) Ishida & Weinberger (1987); (3) Kerber et al. (2000b); (4) Jacoby & Van de Steene (1995); (5) Jacoby et al. (1997); (6) Kohoutek (1962); (7) Kerber et al. (1998); (8) Kerber et al. (2000a); (9) Melmer & Weinberger (1990); (10) Vauclair et al. (1998); (11) Pierce et al. (2004); (12) Rauch et al. (2004); (13) Tweedy & Kwitter (1996); (14) Borkowski et al. (1990).
References for IPNe Expansion Velocity: (1) ESO-Strasburg Catalog; (2) Weinberger (1989); (3) Meaburn et al. (1998); (4) Rodríguez et al. (2001); (5) Pottasch (1996); (6) Guerrero et al. (1998); (7) Phillips (1984); (8) Sabbadin (1984); (9) Hippelein & Weinberger (1990).
© ESO, 2012
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