2013MNRAS.433.1588S

Query : 2013MNRAS.433.1588S

2013MNRAS.433.1588S - Mon. Not. R. Astron. Soc., 433, 1588-1598 (2013/August-1)

CI Aql: a Type Ia supernova progenitor ?

SAHMAN D.I., DHILLON V.S., MARSH T.R., MOLL S., THOROUGHGOOD T.D., WATSON C.A. and LITTLEFAIR S.P.

Abstract (from CDS):

If recurrent novae are progenitors of Type Ia supernovae, their white dwarfs must have masses close to the Chandrasekhar limit. The most reliable means of determining white dwarf masses in recurrent novae is dynamically, via radial-velocity and rotational-broadening measurements of the companion star. Such measurements require the system to be both eclipsing and to show absorption features from the secondary star. Prior to the work reported here, the only dynamical mass estimate of a recurrent nova was for U Sco, which has a white dwarf mass of 1.55±0.24M☉.

We present new time-resolved, intermediate-resolution spectroscopy of the eclipsing recurrent nova CI Aquilae (CI Aql) during quiescence. We find the mass of the white dwarf to be 1.00 ± 0.14M☉ and the mass of the secondary star to be 2.32±0.19M☉. We estimate the radius of the secondary to be 2.07±0.06 R☉, implying that it is a slightly evolved early A-type star. The high mass ratio of q = 2.35±0.24 and the high secondary-star mass implies that the mass transfer occurs on a thermal time-scale. We suggest that CI Aql is rapidly evolving into a supersoft X-ray source, and ultimately may explode as a Type Ia supernova within 10 Myr.


Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)

Journal keyword(s): binaries: eclipsing - binaries: spectroscopic - stars: individual: CI Aql - novae, cataclysmic variables - supernovae: general

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 SN 2011fe SN* 14 03 05.711 +54 16 25.22   10.12 10.06     SNIa-norm 747 1
2 M 101 GiP 14 03 12.583 +54 20 55.50   8.46 7.86 7.76   ~ 3138 2
3 V* U Sco CV* 16 22 30.7791646104 -17 52 43.166822628           F8+K2 592 0
4 UCAC4 443-085347 CV* 18 52 03.5647256952 -01 28 39.190318140       13.373   ~ 176 0

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