2012A&A...543A..85H


Query : 2012A&A...543A..85H

2012A&A...543A..85H - Astronomy and Astrophysics, volume 543A, 85-85 (2012/7-1)

A peculiar of star in the local group galaxy IC 1613.

HERRERO A., GARCIA M., PULS J., UYTTERHOEVEN K., NAJARRO F., LENNON D.J. and RIVERO-GONZALEZ J.G.

Abstract (from CDS):

Result. from the theory of radiatively driven winds are nowadays incorporated in stellar evolutionary and population synthesis models, and are used in our interpretation of the observations of the deep Universe. Yet, the theory has been confirmed only until Small Magellanic Cloud metallicities. Observations and analyses of O-stars at lower metallicities are difficult, but much needed to prove the theory. We have observed GHV-62024, an O6.5 IIIf star in the low-metallicity galaxy IC1613 (Z≃0.15Z) to study its evolution and wind. According to a previous preliminary analysis that was subject to significant restrictions this star could challenge the radiatively driven wind theory at low metallicities. Here we present a complete analysis of this star. Our observations were obtained with VIMOS at VLT, at R≃2000 and covered approximately between 4000 and 7000Å. The observations were analysed using the latest version of the model atmosphere code FASTWIND, which includes the possibility of calculating the NIII spectrum. We obtain the stellar parameters and conclude that the star follows the average wind momentum-luminosity relationship (WLR) expected for its metallicity, but with a high value for the exponent of the wind velocity law, β. Comparing this with values of other stars in the literature, we suggest that this high value may be reached because GHV-62024 could be a fast rotator seen at a low inclination angle. We also suggest that this could favour the appearance of the spectral ``f''-characterictics. While the derived β value does not change by adopting a lower wind terminal velocity, we show that a wrong V has a clear impact on the position of the star in the WLR diagram. The N and He abundances are very high, consistent with strong CNO mixing that could have been caused by the fast rotation, although we cannot discard a different origin with present data. Stellar evolutionary model predictions are consistent with the star being still a fast rotator. We find again the well-known mass-discrepancy for this star. We conclude that the star follows the WLR expected for its metallicity. The results are consistent with GHV-62024 being a fast rotator seen close to pole-on, strongly contaminated at the surface with CNO products and with a wind structure altered by the fast rotation but without modifying the global WLR. We suggest that this could be a general property of fast rotators.

Abstract Copyright:

Journal keyword(s): galaxies: individual: IC1613 - stars: early-type - stars: fundamental parameters - stars: mass-loss - stars: rotation - stars: evolution

Simbad objects: 16

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Number of rows : 16
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 NGC 55 GiG 00 14 53.602 -39 11 47.86 8.54 8.58 7.87 7.84   ~ 765 2
2 AzV 83 s*b 00 50 52.0015192368 -72 42 14.940550980 12.233 13.244 13.366   13.67 O7Iaf+ 47 0
3 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 10843 1
4 NGC 300 GiG 00 54 53.4465638304 -37 41 03.168402396 8.83 8.69 8.13 7.46   ~ 1460 2
5 NGC 346 Cl* 00 59 04.4000 -72 10 39.000           ~ 479 0
6 AzV 226 * 00 59 20.7295412880 -72 17 10.615804836 12.97 14.12 14.19     O7IIIn((f)) 25 0
7 SK 80 s*b 00 59 31.9751731656 -72 10 46.106730444   12.12 12.31     O7Iaf+ 108 0
8 AzV 296 * 01 02 08.6480463408 -72 13 20.012601648 13.01 14.19 14.38   14.62 O7.5V((f)) 17 0
9 IC 1613 GiC 01 04 54.2 +02 08 00   10.42 10.01 9.77   ~ 1206 2
10 [GHV2009] Star 62024 * 01 05 00.646 +02 08 49.26           O6.5III 3 0
11 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 6825 1
12 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 16981 1
13 RMC 136 Cl* 05 38 42.396 -69 06 03.36           ~ 1955 1
14 NGC 3109 G 10 03 06.877 -26 09 34.46 11.10 10.42 10.04 9.91   ~ 756 2
15 NGC 3621 AGN 11 18 16.300 -32 48 45.36 10.10 9.44 9.56 8.07 10.1 ~ 567 3
16 NAME Local Group GrG ~ ~           ~ 8149 0

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2023.09.26-15:41:28

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