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).