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An infrared view of NGC3603

Published online by Cambridge University Press:  29 August 2024

Raúl Castellanos Open the ORCID record for Raúl Castellanos [Opens in a new window] ,
Francisco Najarro ,
Miriam Garcia ,
Lee R. Patrick ,
Christopher J. Evans ,
Elizabeth S. Bartlett  and
J. S. Clark
Raúl Castellanos*
Affiliation:
Centro de Astrobiología, CSIC-INTA, Carretera de Ajalvir km4, 28850 Torrejón de Ardoz, Madrid, Spain.
Francisco Najarro
Affiliation:
Centro de Astrobiología, CSIC-INTA, Carretera de Ajalvir km4, 28850 Torrejón de Ardoz, Madrid, Spain.
Miriam Garcia
Affiliation:
Centro de Astrobiología, CSIC-INTA, Carretera de Ajalvir km4, 28850 Torrejón de Ardoz, Madrid, Spain.
Lee R. Patrick
Affiliation:
Centro de Astrobiología, CSIC-INTA, Carretera de Ajalvir km4, 28850 Torrejón de Ardoz, Madrid, Spain. Departamento de Física Aplicada, Universidad de Alicante, E-03690 San Vicente del Raspeig, Alicante, Spain. School of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK76AA, UK.
Christopher J. Evans
Affiliation:
European Space Agency (ESA), ESA Office, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA.
Elizabeth S. Bartlett
Affiliation:
UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh, UK, EH9 3HJ.
*
email: [email protected]
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Abstract

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NGC3603 is one of the youngest massive clusters of the Milky Way which uniquely enables studying the interplay between massive star feedback and the surrounding interstellar medium. Yet, a deep infrared (IR) view of the cluster is missing. We present guaranteed time observations of NGC3603 consisting of near infrared spectroscopy taken with VLT-KMOS. This data set will provide a first, rather complete IR census.

Keywords

stars: early-typegalaxies: star clustersopen clusters and associations: individual (NGC3603)
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 97 - 99
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Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

Footnotes

†

The author is deceased.

References

Drew, J. E., Monguió, M., & Wright, N. J. 2019, MNRAS, 486, 1034 Google Scholar
Harayama, Y., Eisenhauer, F., & Martins, F. 2008, ApJ, 675, 1319 Google Scholar
Hillier, D. J., & Miller, D. L. 1998, ApJ, 496, 407 Google Scholar
Kalari, V. M., Vink, J. S., de Wit, W. J., Bastian, N. J., & Méndez, R. A. 2019, A&A, 625, L2 Google Scholar
Melena, N. W., Massey, P., Morrell, N. I., & Zangari, A. M. 2008, AJ, 135, 878 CrossRefGoogle Scholar
Melnick, J., Tapia, M., & Terlevich, R. 1989, A&A, 213, 89 Google Scholar
Moffat, A. F. J. 1983, A&A, 124, 273 Google Scholar
Roman-Lopes, A., Franco, G. A. P., & Sanmartim, D. 2016, ApJ, 823, 96 CrossRefGoogle Scholar
Smette, A., et al. 2015, A&A, 576, A77 Google Scholar