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Hot subdwarf wind models with accurate abundances I. Hydrogen dominated stars HD 49798 and BD+18° 2647
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| DOI | 10.1051/0004-6361/201936208 | ||||
| Año | 2019 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. Wind models with accurate abundances provide more reliable wind parameters, but the influence of abundances on the wind parameters is limited in many cases.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Krticka, J. | Hombre |
Masarykova Univ - República Checa
Masaryk University - República Checa |
| 2 | Janik, Jan | - |
Masarykova Univ - República Checa
Masaryk University - República Checa |
| 3 | Krtickova, I. | - |
Masarykova Univ - República Checa
Masaryk University - República Checa |
| 4 | Mereghetti, S. | Hombre |
Ist Astrofis Spaziale & Fis Cosm Milano - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia |
| 5 | Pintore, F. | - |
Ist Astrofis Spaziale & Fis Cosm Milano - Italia
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia |
| 6 | Nemeth, P. | Hombre |
Akad Ceske Republiky - República Checa
Academy of Sciences of the Czech Republic - República Checa |
| 7 | Kubat, J. | - |
Akad Ceske Republiky - República Checa
Academy of Sciences of the Czech Republic - República Checa |
| 8 | Vuckovic, Maja | Mujer |
Universidad de Valparaíso - Chile
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| Fuente |
|---|
| National Science Foundation |
| Ministerio de Economía y Competitividad |
| Spanish MINECO |
| ASI-INAF |
| H2020 Marie Skłodowska-Curie Actions |
| Horizon 2020 Framework Programme |
| NOAO |
| Spanish Virtual Observatory |
| European Union's Framework Programme for Research and Innovation Horizon 2020 (2014-2020) under the Marie Sklodowska-Curie grant |
| grant GACR |
| CESNET |
| European Union’s Frame-work Programme for Research and Innovation Horizon 2020 |
| CERIT Scientific Cloud |
| Agradecimiento |
|---|
| This research was supported by grant GACR 18-05665S. SM acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.0. This project has received funding from the European Union's Framework Programme for Research and Innovation Horizon 2020 (2014-2020) under the Marie Sklodowska-Curie grant Agreement No. 823734. Computational resources were provided by the CESNET LM2015042 and the CERIT Scientific Cloud LM2015085, provided under the programme "Projects of Large Research, Development, and Innovations Infrastructures". The Astronomical Institute Ondrejov is supported by the project RVO:67985815. This publication makes use of VOSA, developed under the Spanish Virtual Observatory project supported from the Spanish MINECO through grant AyA2017-84089. |
| 1 IRAF is distributed by NOAO, which is operated by AURA, Inc., under cooperative agreement with the National Science Foundation. 2 Mikulski Archive for Space Telescopes, http://archive.stsci. edu |
