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The massive stellar population of IC 10

Published online by Cambridge University Press:  30 October 2019

Luis J. Corral ,
Miriam García Open the ORCID record for Miriam García [Opens in a new window] ,
Silvana G. Navarro  and
Artemio Herrero
Luis J. Corral
Affiliation:
Intituto de Astronomía y Meteorología, Universidad de Guadalajara, Av. Vallarta 2602, Guadalajara, 44130, Mexico, emails: [email protected], [email protected]
Miriam García
Affiliation:
Centro de Astrobiología (CSIC/INTA), Instituto Nacional de Técnica Aeroespacial, Ctra. de Torrejón de Ajalvir, km 4, E-28850, Madrid, Spain, email: [email protected]
Silvana G. Navarro
Affiliation:
Intituto de Astronomía y Meteorología, Universidad de Guadalajara, Av. Vallarta 2602, Guadalajara, 44130, Mexico, emails: [email protected], [email protected]
Artemio Herrero
Affiliation:
Instituto de Astrofísica de Canarias, C/ Vía Láctea s/n, E-38205 La Laguna, Tenerife, Spain, email: [email protected]
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Abstract

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Using photometric data available in the literature we want to identify the massive stars members of the metal-poor irregular galaxy IC 10 and the clusters and associations that they form. The census of the clusters and associations of these objects is needed to provide information about age and environment on this galaxy that is apparently going through a starburst phase.

Keywords

stars: early-typegalaxies: irregularstellar populationstarburst
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S344: Dwarf Galaxies: From the Deep Universe to the Present , August 2018 , pp. 57 - 61
Copyright
© International Astronomical Union 2019 

References

Battinelli, P., 1991, A&A, 244, 69 Google Scholar
Corral, L. J., Garcia, M., et al., 2019 in preparation Google Scholar
Dolphin, A. E., Saha, A., Skillman, E. D., et al. 2001, ApJ, 550, 554 CrossRefGoogle Scholar
Garcia, M., Herrero, A., Vicente, B., Castro, N., Corral, L. J., Rosenberg, A., & Monelli, M., 2009, A&A, 502, 1015 Google Scholar
Garcia, M., Herrero, A., Castro, N., Corral, L. J., & Rosenberg, A., 2010, A&A, 523, A23 Google Scholar
Garnett, D.R., 1990, ApJ, 363, 142 CrossRefGoogle Scholar
Kim, M., Kim, E., Hwang, N., Lee, M. G., Im, M., Karoji, H., Noumaru, J., & Tanaka, I., 2009, ApJ, 703, 816 CrossRefGoogle Scholar
Lee, M. G., Freedman, W. L., & Madore, B. F. 1993, ApJ, 417, 553 CrossRefGoogle Scholar
Lejeune, T., & Schaerer, D. 2001, A&A, 366, 538 Google Scholar
Massey, P. & Armandroff, T. E., 1995, AJ, 109, 2470 CrossRefGoogle Scholar
Massey, P., Olsen, K. A. G., Hodge, P. W., Jacoby, G. H., McNeill, R. T., Smith, R. C., & Strong, S. B., 2007, AJ, 133, 2393 CrossRefGoogle Scholar
Massey, P., Waterhouse, E., & DeGioia-Eastwood, K., 2000, AJ, 119, 2214 CrossRefGoogle Scholar
Motte, F., Nony, T., Louvet, F., et al., 2018, Nature Astronomy 2, 478.CrossRefGoogle Scholar
Schneider, F. R. N., Sana, H., Evans, C. J. et al., 2018, Science, 359, 69 CrossRefGoogle Scholar