...
首页> 外文期刊>Astronomy and astrophysics >An HST/WFPC2 survey of bright young clusters in M31 - I. VdB0, a massive star cluster seen at t $simeq$ 25 Myr
【24h】

An HST/WFPC2 survey of bright young clusters in M31 - I. VdB0, a massive star cluster seen at t $simeq$ 25 Myr

机译:HST / WFPC2对M31中明亮的年轻星团-I. VdB0的调查,这是一个质量大的星团,其观测值为t simeq $ 25 Myr

获取原文
   

获取外文期刊封面封底 >>

       

摘要

Aims. We introduce our imaging survey of possible young massive globular clusters in M31 performed with the Wide Field and Planetary Camera2 (WFPC2) on the Hubble Space Telescope (HST). We obtained shallow (to )photometry of individual stars in 20candidate clusters. We present here details of the data reduction pipeline that is being applied to all the survey data and describe its application to the brightest among our targets, van den Bergh0 (VdB0), taken as a test case. Methods. Point spread function fitting photometry of individual stars was obtained for all the WFPC2images of VdB0 and the completeness of the final samples was estimated using an extensive set of artificial stars experiments. The reddening, the age and the metallicity of the cluster were estimated by comparing the observed color magnitude diagram (CMD) with theoretical isochrones. Structural parameters were obtained from model-fitting to the intensity profiles measured within circular apertures on the WFPC2images. Results. Under the most conservative assumptions, the stellar mass of VdB0 is M> 2.4,but our best estimates lie in the range 4-9.The CMD of VdB0 is best reproduced by models having solar metallicity and age25Myr. Ages less than 12Myr and greater than 60Myr are clearly ruled out by the available data. The cluster has a remarkable number of red super giants (18) and a CMD very similar to Large Magellanic Cloud clusters usually classified as young globulars such as NGC1850, for example. Conclusions. VdB0 is significantly brighter (1mag) than Galactic open clusters of similar age. Its present-day mass and half-light radius (pc) are more typical of faint globular clusters than of open clusters. However, given its position within the disk of M31, it is expected to be destroyed by dynamical effects, in particular by encounters with giant molecular clouds, within the next 4Gyr. Key words: galaxies: star clusters - galaxies: individual: M31 - stars: supergiants - stars: evolution
机译:目的我们介绍了在哈勃太空望远镜(HST)上使用广角和行星照相机2(WFPC2)对M31中可能存在的年轻块状球状星团进行的成像调查。我们获得了20个候选星团中单个恒星的浅(至)光度法。我们在这里介绍了将应用于所有调查数据的数据缩减管道的详细信息,并描述了它在我们的目标中最亮的目标van den Bergh0(VdB0)(作为测试用例)中的应用。方法。对于VdB0的所有WFPC2图像,获得了单个恒星的点扩散函数拟合光度法,并使用大量的人造恒星实验对最终样品的完整性进行了估计。通过将观察到的色度图(CMD)与理论等时线进行比较,可以估算出团簇的变红,寿命和金属性。结构参数是通过对WFPC2图像上圆形孔内测得的强度分布进行模型拟合获得的。结果。在最保守的假设下,VdB0的恒星质量为M> 2.4,但我们的最佳估算值在4-9范围内。VdB0的CMD最好由具有太阳金属性和25Myr年龄的模型重现。可用数据明确排除了小于12岁且大于60岁的年龄。该星团有大量红色超巨星(18),其CMD与通常被归类为年轻球状的大型麦哲伦星团(如NGC1850)非常相似。结论。 VdB0比类似年龄的银河系开放星团亮得多(1mag)。它的当前质量和半光半径(pc)在微弱的球状星团中比在开放星团中更典型。但是,考虑到它在M31盘中的位置,预计它会在下一个4Gyr内因动力学效应而被破坏,尤其是遇到巨大的分子云时会被破坏。关键词:星系:星团-星系:个体:M31-恒星:超巨星-恒星:演化

著录项

相似文献

  • 外文文献
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号