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Astro+: Design, construction, and scientific exploitation of a large-scale massive star spectroscopic database

Published online by Cambridge University Press:  29 August 2024

Klaus Rübke ,
Amparo Marco ,
Ignacio Negueruela ,
Artemio Herrero ,
Sergio Simon-Diaz ,
Hugo Tabernero  and
Lee Patrick
Klaus Rübke*
Affiliation:
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig, Spain
Amparo Marco
Affiliation:
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig, Spain
Ignacio Negueruela
Affiliation:
Departamento de Física Aplicada, Facultad de Ciencias, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig, Spain
Artemio Herrero
Affiliation:
Instituto de Astrofísica de Canarias, Vía Láctea s/n, E38200, La Laguna, Tenerife, Spain Universidad de La Laguna, Departamento de Astrofísica, E38206 La Laguna, Tenerife, Spain
Sergio Simon-Diaz
Affiliation:
Instituto de Astrofísica de Canarias, Vía Láctea s/n, E38200, La Laguna, Tenerife, Spain Universidad de La Laguna, Departamento de Astrofísica, E38206 La Laguna, Tenerife, Spain
Hugo Tabernero
Affiliation:
Centro de Astrobiología, CSIC-INTA. Campus ESAC. C. bajo del castillo s/n. E-28 692 Villanueva de la Cañada, Madrid, Spain
Lee Patrick
Affiliation:
Departamento de Física Aplicada, Facultad de Ciencias, Universidad de Alicante, Carretera de San Vicente s/n, E03690, San Vicente del Raspeig, Spain School of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK
*
email: klaus.rubke@ua.es
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Abstract

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Massive stars are the objects that condition the evolution of the interstellar medium by the amount of energy released during their lives and especially by their death as a supernova explosion. All the data provided by the previous and ongoing missions of ground and space telescopes have saturated us with the amount of information, which is no longer easy to process daily by human routines. To this end, we present the development of a massive star spectroscopic interactive database designed for scientific research.

Keywords

DatabaseMassive-starsAutomatic-programsparameter-determination
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 197 - 199
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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

References

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