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Alicante Survey of Massive Stars in H ii regions (A-SMASHER)

Published online by Cambridge University Press:  29 August 2024

A. Marco*
Affiliation:
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, EPS, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig, Spain
I. Negueruela
Affiliation:
Departamento de Física Aplicada, Facultad de Ciencias, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig, Spain
D. de la Fuente
Affiliation:
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, EPS, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig, Spain CREOL, The College of Optics and Photonics, University of Central Florida, USA
L. R. Patrick
Affiliation:
Departamento de Física Aplicada, Facultad de Ciencias, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig, Spain
A. Herrero
Affiliation:
Instituto de Astrofísica de Canarias, Vía Láctea s/n, E38200, La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de la Laguna, Avenida Astrofsico Francisco Sánchez, s/n, Facultad de Ciencias, E38200, La Laguna, Tenerife, Spain
S. S. Eikenberry
Affiliation:
CREOL, The College of Optics and Photonics, University of Central Florida, USA
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Abstract

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The aim of this survey is the homogeneous characterization of a large sample of H ii regions with active star formation in order to detect observational trends supporting the two main models of massive star formation.

Type
Poster Paper
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

Krumholz, et al. 2009, Science, 323, 754 CrossRefGoogle Scholar
Bonnell & Bate, 2006, MNRAS, 370, 488 CrossRefGoogle Scholar
de la Fuente et al. 2022, Proceedings IAU Symposium No. 361, 2022Google Scholar
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