Dataciencia

Colección SciELO Chile

HR 6819 is a binary system with no black hole Revisiting the source with infrared interferometry and optical integral field spectroscopy

Indexado

WoS	WOS:000763012500008
Scopus	SCOPUS_ID:85126130901

DOI

10.1051/0004-6361/202143004

Año

2022

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. We conclude that HR 6819 is a binary system and that no BH is present in the system. The unique nature of HR 6819, and its proximity to Earth make it an ideal system for quantitatively characterising the immediate outcome of binary interaction and probing how Be stars form.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

Métricas Externas

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Frost, A. J.	-	Katholieke Univ Leuven - Bélgica KU Leuven - Bélgica
2	Bodensteiner, J.	Mujer	Observatorio Europeo Austral - Alemania
3	Rivinius, Th	Hombre	Observatorio Europeo Austral - Chile Observatorio Europeo Austral - Alemania European Southern Observatory Santiago - Chile
4	Baade, D.	Hombre	Observatorio Europeo Austral - Alemania
5	Merand, Antoine	Hombre	Observatorio Europeo Austral - Alemania
6	Selman, Fernando	Hombre	Observatorio Europeo Austral - Chile Observatorio Europeo Austral - Alemania European Southern Observatory Santiago - Chile
7	Abdul-Masih, M.	Hombre	Observatorio Europeo Austral - Chile Observatorio Europeo Austral - Alemania European Southern Observatory Santiago - Chile
8	Banyard, G.	-	Katholieke Univ Leuven - Bélgica KU Leuven - Bélgica
9	Bordier, E.	-	Katholieke Univ Leuven - Bélgica Observatorio Europeo Austral - Chile KU Leuven - Bélgica Observatorio Europeo Austral - Alemania European Southern Observatory Santiago - Chile
10	Dsilva, K.	-	Katholieke Univ Leuven - Bélgica KU Leuven - Bélgica
11	Hawcroft, Calum	-	Katholieke Univ Leuven - Bélgica KU Leuven - Bélgica
12	Mahy, L.	Hombre	Royal Observ Belgium - Bélgica Royal Observatory of Belgium - Bélgica
13	Reggiani, M.	Mujer	Katholieke Univ Leuven - Bélgica KU Leuven - Bélgica
14	Shenar, T.	Hombre	Univ Amsterdam - Países Bajos Anton Pannekoek Instituut voor Sterrenkunde - Países Bajos
15	CABEZAS-RETAMAL, MAURICIO EDUARDO	Hombre	Acad Sci Czech Republ - República Checa Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i. - República Checa
16	Hadrava, P.	Hombre	Acad Sci Czech Republ - República Checa Astronomical Institute, Academy of Sciences of the Czech Republic v.v.i. - República Checa
17	Heida, Marianne	Mujer	Observatorio Europeo Austral - Alemania
18	Klement, Robert	Hombre	Georgia State Univ - Estados Unidos Georgia State University - Estados Unidos
19	Sana, H.	Hombre	Katholieke Univ Leuven - Bélgica KU Leuven - Bélgica

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Financiamiento

Fuente
European Research Council
ESO Fellowship
European Research Council (ERC) under the European Union
European School of Oncology
Horizon 2020 Framework Programme
Marie Sklodowska-Curie
European Union's Horizon 2020 under the Marie Sklodowska-Curie grant

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Agradecimientos

Agradecimiento
We thank Dr. Jesus Maiz Appellaniz for his helpful and thoughtful comments as referee. This research has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement number 772225: MULTIPLES). J.B. and M.H. are supported by an ESO fellowship. T.S. acknowledges funding received from the European Union's Horizon 2020 under the Marie Sklodowska-Curie grant agreement No. 101024605. We also thank the team behind QFitsView for developing their tool which allowed easy handling of our MUSE data.
Acknowledgements. We thank Dr. Jesús Maíz Appellániz for his helpful and thoughtful comments as referee. This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement number 772225: MULTIPLES). J.B. and M.H. are supported by an ESO fellowship. T.S. acknowledges funding received from the European Union’s Horizon 2020 under the Marie Skłodowska-Curie grant agreement No. 101024605. We also thank the team behind QFitsView for developing their tool which allowed easy handling of our MUSE data.

Agradecimiento

We thank Dr. Jesus Maiz Appellaniz for his helpful and thoughtful comments as referee. This research has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement number 772225: MULTIPLES). J.B. and M.H. are supported by an ESO fellowship. T.S. acknowledges funding received from the European Union's Horizon 2020 under the Marie Sklodowska-Curie grant agreement No. 101024605. We also thank the team behind QFitsView for developing their tool which allowed easy handling of our MUSE data.

Acknowledgements. We thank Dr. Jesús Maíz Appellániz for his helpful and thoughtful comments as referee. This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement number 772225: MULTIPLES). J.B. and M.H. are supported by an ESO fellowship. T.S. acknowledges funding received from the European Union’s Horizon 2020 under the Marie Skłodowska-Curie grant agreement No. 101024605. We also thank the team behind QFitsView for developing their tool which allowed easy handling of our MUSE data.