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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

New eclipsing binaries with mercury-manganese stars

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Autor(es):
Kochukhov, O. [1] ; Labadie-Bartz, J. [2] ; Khalack, V [3] ; Shultz, M. E. [4]
Número total de Autores: 4
Afiliação do(s) autor(es):
[1] Uppsala Univ, Dept Phys & Astron, POB 516, SE-75120 Uppsala - Sweden
[2] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, Rua Matao 1226, Cidade Univ, BR-05508900 Sao Paulo, SP - Brazil
[3] Univ Moncton, Dept Phys & Astron, Moncton, NB E1A 3E9 - Canada
[4] Univ Delaware, Dept Phys & Astron, Sharp Lab 217, Newark, DE 19716 - USA
Número total de Afiliações: 4
Tipo de documento: Artigo Científico
Fonte: Monthly Notices of the Royal Astronomical Society; v. 506, n. 1, p. L40-L44, SEP 2021.
Citações Web of Science: 1
Resumo

Eclipsing binary stars are rare and extremely valuable astrophysical laboratories that make possible precise determination of fundamental stellar parameters. Investigation of early-type chemically peculiar stars in eclipsing binaries provides important information for understanding the origin and evolutionary context of their anomalous surface chemistry. In this study, we discuss observations of eclipse variability in six mercury-manganese (HgMn) stars monitored by the Transiting Exoplanet Survey Satellite (TESS) satellite. These discoveries double the number of known eclipsing HgMn stars and yield several interesting objects requiring further study. In particular, we confirm eclipses in HD 72208, thereby establishing this object as the longestperiod eclipsing HgMn star. Among five other eclipsing binaries, reported here for the first time, HD 36892 and HD 53004 stand out as eccentric systems showing heartbeat variability in addition to eclipses. The latter object has the highest eccentricity among eclipsing HgMn stars and also exhibits tidally induced oscillations. Finally, we find evidence that HD 55776 may be orbited by a white dwarf companion. (AU)

Processo FAPESP: 17/23731-1 - Análise e Modelagem de uma Grande Amostra de Estrelas Be Galácticas
Beneficiário:Jonathan Michael Labadie-Bartz
Modalidade de apoio: Bolsas no Brasil - Pós-Doutorado