Study of the low-order Delta nu-(rho)over-bar relation for moderately rotating delta Scuti stars and its impact on their characterization

Monthly Notices of the Royal Astronomical Society(2020)

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摘要
The authors acknowledge funding support from Spanish public funds (including FEDER funds) for research under projects ESP2017-87676-C5-2-R, ESP2017-87676-C5-5-R, and PID2019107061GB-C64. Julio E. Rodriguez-Mart \u0027 in also acknowledges financial support from the State Agency for Research of the Spanish Ministerio de Ciencia, Innovacion y Universidades through the \u0027Center of Excellence Severo Ochoa\u0027 award to the Instituto de Astrof \u0027 isica de Andalucia-Consejo Superior de Investigaciones Cient \u0027 ificas (SEV2017-0709). Antonio Garcia Hernandez also acknowledges support from `Fondo Europeo de Desarrollo Regional/Junta de AndaluciaConsejeria de Economia y Conocimiento\u0027 under project E-FQM041-UGR18 by Universidad de Granada. Juan Carlos Suarez also acknowledges support from project RYC-2012-09913 under the \u0027Ramon y Cajal\u0027 programme of the Spanish Ministry of Science and Education. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.e sa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC; https://www.cosmos.esa.int/web/gaia/dpac/con sortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.
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关键词
stars: oscillations,stars: rotation,stars: variables: Scuti
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