TY - GEN
T1 - A barium-rich binary central star in Abell 70
AU - Boffin, Henri M J
AU - Miszalski, Brent
AU - Frew, David J.
AU - Acker, Agnes
AU - Köppen, Joachim
AU - Moffat, Anthony F J
AU - Parker, Quentin A.
PY - 2011/7
Y1 - 2011/7
N2 - We have found the central star of Abell 70 (PN G038.1-25.4, hereafter A 70) to be a binary consisting of a G8 IV-V secondary and a hot white dwarf. The secondary shows enhanced Ba II and Sr II features, firmly classifying it as a barium star. The nebula is found to have Type-I chemical abundances with helium and nitrogen enrichment, which combined with future abundance studies of the central star, will establish A 70 as a unique laboratory for studying s-process AGB nucleosynthesis.
AB - We have found the central star of Abell 70 (PN G038.1-25.4, hereafter A 70) to be a binary consisting of a G8 IV-V secondary and a hot white dwarf. The secondary shows enhanced Ba II and Sr II features, firmly classifying it as a barium star. The nebula is found to have Type-I chemical abundances with helium and nitrogen enrichment, which combined with future abundance studies of the central star, will establish A 70 as a unique laboratory for studying s-process AGB nucleosynthesis.
KW - binaries: general
KW - binaries: symbiotic
KW - planetary nebulae: general
KW - planetary nebulae: individual (PN G038.1-25.4)
KW - stars: AGB and post-AGB
KW - stars: chemically peculiar
UR - http://www.scopus.com/inward/record.url?scp=84865760336&partnerID=8YFLogxK
U2 - 10.1017/S1743921312011192
DO - 10.1017/S1743921312011192
M3 - Conference proceeding contribution
AN - SCOPUS:84865760336
SN - 9781107019836
VL - 7
T3 - Proceedings of the International Astronomical Union
SP - 314
EP - 315
BT - Planetary Nebulae: An Eye to the Future
A2 - Manchado, Arturo
A2 - Stanghellini, Letizia
A2 - Schönberner, Detlef
CY - Cambridge, UK
ER -