Pulsation in the white dwarf HE 1017−1352
Autor(a) principal: | |
---|---|
Data de Publicação: | 2020 |
Outros Autores: | , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/223015 |
Resumo: | We report the detection of periodic variations on the Teff 32 000 K DA white dwarf star HE 1017−1352. We obtained time series photometry using the 4.1-m Southern Astrophysical Research telescope on three separate nights for a total of 16.8 h. From the frequency analysis, we found four periods of 605, 556, 508, and 869 s with significant amplitudes above the 1/1000 false alarm probability detection limit. The detected modes are compatible with low harmonic degree g-mode non-radial pulsations with radial order higher than ∼9. This detection confirms the pulsation nature of HE 1017−1352 and thus the existence of the new pulsating class of hot DA white dwarf stars. In addition, we detect a long period of 1.52 h, compatible with a rotation period of DA white dwarf stars. |
id |
UFRGS-2_e199c660932abed9bb14ee8003f14781 |
---|---|
oai_identifier_str |
oai:www.lume.ufrgs.br:10183/223015 |
network_acronym_str |
UFRGS-2 |
network_name_str |
Repositório Institucional da UFRGS |
repository_id_str |
|
spelling |
Romero, Alejandra DanielaAmaral, Larissa AntunesKepler, Souza OliveiraFraga, LucianoKurtz, Donald W.Shibahashi, Hiromoto2021-06-30T04:23:24Z20200035-8711http://hdl.handle.net/10183/223015001124301We report the detection of periodic variations on the Teff 32 000 K DA white dwarf star HE 1017−1352. We obtained time series photometry using the 4.1-m Southern Astrophysical Research telescope on three separate nights for a total of 16.8 h. From the frequency analysis, we found four periods of 605, 556, 508, and 869 s with significant amplitudes above the 1/1000 false alarm probability detection limit. The detected modes are compatible with low harmonic degree g-mode non-radial pulsations with radial order higher than ∼9. This detection confirms the pulsation nature of HE 1017−1352 and thus the existence of the new pulsating class of hot DA white dwarf stars. In addition, we detect a long period of 1.52 h, compatible with a rotation period of DA white dwarf stars.application/pdfengMonthly notices of the royal astronomical society. Oxford. Vol. 497, no. 1 (Sep. 2020), p. L24-L29Anãs brancasPulsacoes estelaresEvolucao galaticaStars: interiorsStars: variables: generalWhite dwarfsPulsation in the white dwarf HE 1017−1352Estrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSTEXT001124301.pdf.txt001124301.pdf.txtExtracted Texttext/plain28968http://www.lume.ufrgs.br/bitstream/10183/223015/2/001124301.pdf.txtc80a3b402b17869c19c467b2473dadd3MD52ORIGINAL001124301.pdfTexto completo (inglês)application/pdf2575920http://www.lume.ufrgs.br/bitstream/10183/223015/1/001124301.pdfe844b23a4dad7d8157e48fb5541257ecMD5110183/2230152023-05-14 03:24:05.398819oai:www.lume.ufrgs.br:10183/223015Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-05-14T06:24:05Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Pulsation in the white dwarf HE 1017−1352 |
title |
Pulsation in the white dwarf HE 1017−1352 |
spellingShingle |
Pulsation in the white dwarf HE 1017−1352 Romero, Alejandra Daniela Anãs brancas Pulsacoes estelares Evolucao galatica Stars: interiors Stars: variables: general White dwarfs |
title_short |
Pulsation in the white dwarf HE 1017−1352 |
title_full |
Pulsation in the white dwarf HE 1017−1352 |
title_fullStr |
Pulsation in the white dwarf HE 1017−1352 |
title_full_unstemmed |
Pulsation in the white dwarf HE 1017−1352 |
title_sort |
Pulsation in the white dwarf HE 1017−1352 |
author |
Romero, Alejandra Daniela |
author_facet |
Romero, Alejandra Daniela Amaral, Larissa Antunes Kepler, Souza Oliveira Fraga, Luciano Kurtz, Donald W. Shibahashi, Hiromoto |
author_role |
author |
author2 |
Amaral, Larissa Antunes Kepler, Souza Oliveira Fraga, Luciano Kurtz, Donald W. Shibahashi, Hiromoto |
author2_role |
author author author author author |
dc.contributor.author.fl_str_mv |
Romero, Alejandra Daniela Amaral, Larissa Antunes Kepler, Souza Oliveira Fraga, Luciano Kurtz, Donald W. Shibahashi, Hiromoto |
dc.subject.por.fl_str_mv |
Anãs brancas Pulsacoes estelares Evolucao galatica |
topic |
Anãs brancas Pulsacoes estelares Evolucao galatica Stars: interiors Stars: variables: general White dwarfs |
dc.subject.eng.fl_str_mv |
Stars: interiors Stars: variables: general White dwarfs |
description |
We report the detection of periodic variations on the Teff 32 000 K DA white dwarf star HE 1017−1352. We obtained time series photometry using the 4.1-m Southern Astrophysical Research telescope on three separate nights for a total of 16.8 h. From the frequency analysis, we found four periods of 605, 556, 508, and 869 s with significant amplitudes above the 1/1000 false alarm probability detection limit. The detected modes are compatible with low harmonic degree g-mode non-radial pulsations with radial order higher than ∼9. This detection confirms the pulsation nature of HE 1017−1352 and thus the existence of the new pulsating class of hot DA white dwarf stars. In addition, we detect a long period of 1.52 h, compatible with a rotation period of DA white dwarf stars. |
publishDate |
2020 |
dc.date.issued.fl_str_mv |
2020 |
dc.date.accessioned.fl_str_mv |
2021-06-30T04:23:24Z |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10183/223015 |
dc.identifier.issn.pt_BR.fl_str_mv |
0035-8711 |
dc.identifier.nrb.pt_BR.fl_str_mv |
001124301 |
identifier_str_mv |
0035-8711 001124301 |
url |
http://hdl.handle.net/10183/223015 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Monthly notices of the royal astronomical society. Oxford. Vol. 497, no. 1 (Sep. 2020), p. L24-L29 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UFRGS instname:Universidade Federal do Rio Grande do Sul (UFRGS) instacron:UFRGS |
instname_str |
Universidade Federal do Rio Grande do Sul (UFRGS) |
instacron_str |
UFRGS |
institution |
UFRGS |
reponame_str |
Repositório Institucional da UFRGS |
collection |
Repositório Institucional da UFRGS |
bitstream.url.fl_str_mv |
http://www.lume.ufrgs.br/bitstream/10183/223015/2/001124301.pdf.txt http://www.lume.ufrgs.br/bitstream/10183/223015/1/001124301.pdf |
bitstream.checksum.fl_str_mv |
c80a3b402b17869c19c467b2473dadd3 e844b23a4dad7d8157e48fb5541257ec |
bitstream.checksumAlgorithm.fl_str_mv |
MD5 MD5 |
repository.name.fl_str_mv |
Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS) |
repository.mail.fl_str_mv |
|
_version_ |
1798487474323849216 |