How do massive stars form? Finding targets for MIRADAS

Marco, A.; Negueruela, I.; Eikenberry, S. S.; Herrero, A.
Bibliographical reference

Highlights on Spanish Astrophysics X, Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16-20, 2018, in Salamanca, Spain, ISBN 978-84-09-09331-1. B. Montesinos, A. Asensio Ramos, F. Buitrago, R. Schödel, E. Villaver, S. Pérez-Hoyos, I. Ordóñez-Etxeberria (eds.) p. 353-358

Advertised on:
3
2019
Number of authors
4
IAC number of authors
1
Citations
0
Refereed citations
0
Description
Observations from massive stars in H II regions can help to clarify theories of massive star formation because they show the degree of isolation under which massive stars can be formed. We present a new survey, called 'A-SMASHeR', consisting of massive stars associated to not yet characterized H II regions that are either more distant or more heavily embedded than the traditional samples. It will allow us to study in a homogeneus way many massive stars placed at different distances between l=30° and 180°, presenting different reddenings and metallicities. Besides, we will use it to constrain better the theories of stellar formation and design future observations with MIRADAS.