Star Formation as Seen by Low Mass Stars

Authors

  • Nino Panagia Supernova Ltd, OYV #131, Northsound Road, Virgin Gorda, British Virgin Islands
  • Guido De Marchi European Space Agency, Keplerlaan 1, 2200 AG Noordwijk, Netherlands

DOI:

https://doi.org/10.14311/APP.2014.01.0113

Abstract

Using the Hubble Space Telescope (HST) we have characterised and compared the physical properties of a large sample of pre-main sequence (PMS) stars spanning a wide range of masses (0:5 - 4Mʘ), metallicities (0:1 - 1 Zʘ) and ages (0:5 - 30 Myr). This is presently the largest and most homogeneous sample of PMS objects with known physical properties. The main results of this ongoing study are briefly summarised here.

Downloads

Download data is not yet available.

Downloads

Published

2014-12-04

Issue

Vol. 1 No. 1 (2014): FRASCATI WORKSHOP 2013

Section

Articles

How to Cite

Star Formation as Seen by Low Mass Stars. (2014). Acta Polytechnica CTU Proceedings, 1(1), 113-117. https://doi.org/10.14311/APP.2014.01.0113