2011A&A...530L..14B


Query : 2011A&A...530L..14B

2011A&A...530L..14B - Astronomy and Astrophysics, volume 530, L14-14 (2011/6-1)

The VLT-FLAMES Tarantula survey. III. A very massive star in apparent isolation from the massive cluster R136.

BESTENLEHNER J.M., VINK J.S., GRAEFENER G., NAJARRO F., EVANS C.J., BASTIAN N., BONANOS A.Z., BRESSERT E., CROWTHER P.A., DORAN E., FRIEDRICH K., HENAULT-BRUNET V., HERRERO A., DE KOTER A., LANGER N., LENNON D.J., MAIZ-APELLANIZ J., SANA H., SOSZYNSKI I. and TAYLOR W.D.

Abstract (from CDS):

VFTS682 is located in an active star-forming region, at a projected distance of 29pc from the young massive cluster R136 in the Tarantula Nebula of the Large Magellanic Cloud. It was previously reported as a candidate young stellar object, and more recently spectroscopically revealed as a hydrogen-rich Wolf-Rayet (WN5h) star. Our aim is to obtain the stellar properties, such as its intrinsic luminosity, and to investigate the origin of VFTS682. To this purpose, we model optical spectra from the VLT-FLAMES Tarantula Survey with the non-LTE stellar atmosphere code cmfgen, as well as the spectral energy distribution from complementary optical and infrared photometry. We find the extinction properties to be highly peculiar (RV∼4.7), and obtain a surprisingly high luminosity log(L/L)=6.5±0.2, corresponding to a present-day mass of ∼150M. The high effective temperature of 52.2±2.5kK might be explained by chemically homogeneous evolution - suggested to be the key process in the path towards long gamma-ray bursts. Lightcurves of the object show variability at the 10% level on a timescale of years. Such changes are unprecedented for classical Wolf-Rayet stars, and are more reminiscent of Luminous Blue Variables. Finally, we discuss two possibilities for the origin of VFTS682: (i) the star either formed in situ, which would have profound implications for the formation mechanism of massive stars, or (ii) VFTS682 is a slow runaway star that originated from the dense cluster R136, which would make it the most massive runaway known to date.

Abstract Copyright:

Journal keyword(s): stars: Wolf-Rayet - stars: early-type - stars: atmospheres - stars: mass-loss - stars: fundamental parameters

Simbad objects: 11

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Number of rows : 11
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 10194 1
2 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 6276 1
3 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 15989 1
4 NAME 30 Dor Nebula SFR 05 38 36.0 -69 05 11           ~ 1099 2
5 BAT99 106 WR* 05 38 42.291 -69 06 03.45   12.83 12.93     WN5h 56 0
6 RMC 136 Cl* 05 38 42.396 -69 06 03.36           ~ 1857 1
7 HD 269926 WR* 05 38 47.5179121824 -69 00 25.287752196 11.953 12.974 13.116 13.16 12.926 WN4+OB 65 0
8 UCAC4 105-014417 WR* 05 38 55.5222410976 -69 04 26.809579344   16.66 16.08   14.89 WN5h 56 0
9 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 12902 0
10 NAME Arches Cluster Cl* 17 45 50.5 -28 49 28           ~ 685 0
11 WR 102ka WR* 17 46 18.12 -29 01 36.6           WN10 30 0

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2022.05.20-15:18:18

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