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Characterizing star formation in the innermost kiloparsec of the galaxy NGC 1386

Published online by Cambridge University Press:  09 June 2023

Gustavo Bruzual ,
Almudena Prieto ,
C. Gladis Magris Open the ORCID record for C. Gladis Magris [Opens in a new window]  and
Juan A. Fernández-Ontiveros
Gustavo Bruzual
Affiliation:
Instituto de Radioastronomía y Astrofísica, UNAM, México
Almudena Prieto
Affiliation:
Instituto de Astrofísica de Canarias (IAC), E-38200 La Laguna, Tenerife, Spain Dept. Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain
C. Gladis Magris
Affiliation:
Centro de Investigaciones de Astonomía (CIDA), Mérida, Venezuela
Juan A. Fernández-Ontiveros
Affiliation:
Centro de Estudios de Física del Cosmos de Aragón, Plaza San Juan 1, 44001 Teruel, Spain
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Abstract

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We characterize the star formation going on in the inner kiloparsec region of the galaxy NGC 1386 as derived from the analysis of a multiwavelength dataset covering the optical, near-IR and mid-IR at subarsec resolution. We detect 61 point sources, distributed in a ring of 960 pc radius around the center of the galaxy. From SED fitting we conclude that these are low mass () young clusters, with age distributed from 1 to 10 Myr, with median at 3.6 Myr. Comparison of the Hα luminosity of the clusters derived from the Hα+[N ii] narrow band image with that expected from the fitted ionizing continuum shows that a large fraction of the ionizing photons escapes from the clusters. Moreover, a large fraction of these photons escapes from the regions around the star forming ring.

Keywords

galaxies: individual NGC1386galaxies: star formationgalaxies: ISMmethods: data analysis
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 17 , Symposium S373: Resolving the Rise and Fall of Star Formation in Galaxies , August 2021 , pp. 111 - 113
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Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Bressan, A., Marigo, P., Girardi, L., Salasnich, B., Dal Cero, C., Rubele, S., Nanni, A. 2012, MNRAS, 427, 127 CrossRefGoogle Scholar
Bruzual, A. G., 2002, in Geisler, D. P., Grebel, E. K., Minniti, D., eds, Vol. 207, Extragalactic Star Clusters. p. 616 (arXiv:astro-ph/0110245)Google Scholar
Charlot, S., Bruzual, G. 2022, In preparation Google Scholar
Chabrier, G., 2003, PASP, 115, 763 CrossRefGoogle Scholar
Magris, C., G, Mateu, P., J., Mateu, C., Bruzual, A., G., Cabrera-Ziri, I., Mejía-Narváez, A.. 2015,. PASP, 127, 16 CrossRefGoogle Scholar
Turner, J.A. et al. 2021, MNRAS, 502, 1366 CrossRefGoogle Scholar
Prieto, M.A., Fernandez-Ontiveros, J.A., Bruzual, G., Burkert, A., Schartmann, M., Charlot, S., 2019, MNRAS, 485, 3264 CrossRefGoogle Scholar
Prieto, M.A. et al 2022, In preparation Google Scholar