Abstract Details
Name: ANAND MY Affiliation: Jawaharalal Nehru Planetarium, Bangalore Conference ID: ASI2019_303 Title : A study of wind blown bubble around HD 148937 Authors and Co-Authors : M.Y.ANAND, B.A. Kagali Abstract Type : Poster Abstract Category : Stars, ISM and Galaxy Abstract : HD148937 is a massive early type star surrounded by ellipsoidal filamentary nebulosity interpreted as a stellar windblown bubble. This study has been made using IUE high resolution spectra which shows many singly ionised dominant species like Si II, Fe II and others, also highly ionised species like Al III and CIV have been seen in the spectra. Estimated radial velocity of these line, have been identified with the swept up region around the HD148937. From the study we have derived the age of the bubble to be 1.31x10^5 years, which is less than the age of the central star (3-4 Myr). |