Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-25T23:35:28.887Z Has data issue: false hasContentIssue false
  • English
  • Français

Ultraviolet observations of massive stars and the instrumentation to come

Published online by Cambridge University Press:  29 August 2024

Ana I. Gómez de Castro Open the ORCID record for Ana I. Gómez de Castro [Opens in a new window]
Ana I. Gómez de Castro*
Affiliation:
Joint Center for Ultraviolet Astronomy, Universidad Complutense de Madrid, Avda. Puerta de Hierro s/n, 28040 Madrid S.D. Fsica de la Tierra y Astrofsica, Fac. CC Matemáticas, Plaza de Ciencias 3, 28040 Madrid
*
email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The wealth of information obtained about massive stars from observations at ultraviolet (UV) wavelengths has been fundamental to understand their structure and the mechanisms regulating their evolution. There are however, important aspects that have not yet been addressed due to the lack of data and the relevant instrumentation such as the role of binarity and magnetic fields or the impact of low metallicity in the evolution of massive stars. There are plans to develop UV spectropolarimeters, UV monitors and very efficient telescopes with high collecting surfaces that will revolutionize the field. In this contribution, a short update on the current and foreseen UV instrumentation is provided.

Keywords

Massive starsultraviolet observationsultraviolet instrumentation.
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 621 - 629
Check for updates
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

Abbott, D.C., 1978, ApJ, 225, 893 Google Scholar
Boggess, A., Carr, F. A., Evans, D. C., et al. 1978, Nature, 275, 372 Google Scholar
Carruthers, G. R., Page, T. 1972, Science, 177, 788 CrossRefGoogle Scholar
Garcia, M., Herrero, A., Najarro, F., et al. 2017, Proc IAU Symp, 329, 313 Google Scholar
Garcia, M. Herrero A., Najarro F., Camacho I., et al. 2019, MNRAS, 484. 422Google Scholar
Gómez de Castro, A.I., Barstow, M.A., Brosch, N., et al. 2021, UV Astronomy and the quest for the origin of life, Elsevier, ISBN:978-0-12-819170-5Google Scholar
Gómez de Castro, A.I., Barstow, M.A., Brosch, N., et al. 2022a, ExpA, 44G, DOI: 10.1007/s10686-022-09854-9 CrossRefGoogle Scholar
Gómez de Castro, A.I., Brosch, N., Bettoni, D. et al. 2022a, ExpA, submittedGoogle Scholar
Kimble, R.A., Woodgate, B.W., Bowers, C.W., et al., 1978, ApJ, 492, L83 Google Scholar
Martin, D. C., Fanson, J., Schiminovich, D., et al. 2005, ApJ, 619, L1 CrossRefGoogle Scholar
Moos, H. W., Cash, W. C., Cowie, L. L., et al. 2000, ApJ, 538, L1 CrossRefGoogle Scholar
Najarro, F., Herrero, A., Verdugo, E., 2006, ApSS, 303, 153 Google Scholar
Rogerson, J. B., Spitzer, L., Drake, J. F., et al. 1973, ApJ, 181, L97 CrossRefGoogle Scholar
Shustov, B., Gómez de Castro, A.I., Sachkov, M., 2022, Proc. of the SPIE, 12181-104Google Scholar
Thilker, D. A., Bianchi, L Meurer, G Gil de Paz, A Boissier, S. et al. 2007, ApJS, 173, 538Google Scholar