Which evolutionary status does the Blue Large-Amplitude Pulsators stay at?-Reference-Cited by-同舟云学术

Which evolutionary status does the Blue Large-Amplitude Pulsators stay at?

Published:2018-05-21 Issue:3 Volume:478 Page:3871-3877
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Wu Tao¹²³^ORCID,Li ¹²³⁴

Affiliation:

1. Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, P. R. China

2. Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, P. R. China

3. Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, P. R. China

4. University of Chinese Academy of Sciences, Beijing 100049, P. R. China

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/478/3/3871/25077249/sty1347.pdf

Reference17 articles.

1. ADIPLS—the Aarhus adiabatic oscillation package

Cited by 21 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Discovery of a new blue large-amplitude pulsator in the SkyMapper DR2: SMSS J184506.82−300804.7;Monthly Notices of the Royal Astronomical Society;2024-03-06

2. The nature of medium-period variables on the extreme horizontal branch;Astronomy & Astrophysics;2024-03

3. OGLE-BLAP-009 – a case study for the properties and evolution of blue large-amplitude pulsators;Monthly Notices of the Royal Astronomical Society;2023-12-20

4. The Formation of Blue Large-amplitude Pulsators from White-dwarf Main-sequence Star Mergers;The Astrophysical Journal;2023-12-01

5. Minute-cadence observations of the LAMOST fields with the TMTS: II. Catalogues of short-period variable stars from the first 2-yr surveys;Monthly Notices of the Royal Astronomical Society;2023-05-30