Abstract Details

Name: Bhagorao Tukaram Tate
Affiliation: Balbhim Arts, science and Commerce College, Beed-431122(M. S) India.
Conference ID: ASI2018_1664
Title : Properties and Fate of Dust in Early type Galaxies
Authors and Co-Authors : B.T. Tate1 M K Patil2 1Department of Physics, Balbhim Arts, Science and Commerce College, Beed 431 122, India 2School of Physical Sciences, S R T M University, Nanded - 431 606, India
Abstract Type : Poster
Abstract Category : Extragalactic astronomy
Abstract : This paper presents multiwavelength analysis of a sample of early-type galaxies with an objective to constrain the origin and properties of dust in this class of galaxies employing high resolution data from HST observatory. It is largely believed that the dust in this class of galaxies has an external origin in the sense that the host has acquired it through the merger like episode. However, it is interesting to see its existence over a long time despite the fact that the dust grains are destructed over a very short timescale due to the thermal sputtering particularly when are embedded within a large fraction of hot gas. This paper further demonstrates that the interstellar dust in these galaxies is not alone due to the external accretion but internal origin is also contributing substantially to the reservoir of its host.