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TESS Cycle 2 observations of roAp stars with 2-min cadence data

Lookup NU author(s): Dr Dominic BowmanORCiD

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This work is licensed under a Creative Commons Attribution 4.0 International License (CC BY 4.0).


Abstract

© The Author(s) 2023.We present the results of a systematic search of the Transiting Exoplanet Survey Satellite (TESS) 2-min cadence data for new rapidly oscillating Ap (roAp) stars observed during the Cycle 2 phase of its mission. We find seven new roAp stars previously unreported as such and present the analysis of a further 25 roAp stars that are already known. Three of the new stars show multiperiodic pulsations, while all new members are rotationally variable stars, leading to almost 70 per cent (22) of the roAp stars presented being α2 CVn-type variable stars. We show that targeted observations of known chemically peculiar stars are likely to overlook many new roAp stars, and demonstrate that multiepoch observations are necessary to see pulsational behaviour changes. We find a lack of roAp stars close to the blue edge of the theoretical roAp instability strip, and reaffirm that mode instability is observed more frequently with precise, space-based observations. In addition to the Cycle 2 observations, we analyse TESS data for all-known roAp stars. This amounts to 18 further roAp stars observed by TESS. Finally, we list six known roAp stars that TESS is yet to observe. We deduce that the incidence of roAp stars amongst the Ap star population is just 5.5 per cent, raising fundamental questions about the conditions required to excite pulsations in Ap stars. This work, coupled with our previous work on roAp stars in Cycle 1 observations, presents the most comprehensive, homogeneous study of the roAp stars in the TESS nominal mission, with a collection of 112 confirmed roAp stars in total.


Publication metadata

Author(s): Holdsworth DL, Cunha MS, Lares-Martiz M, Kurtz DW, Antoci V, Barcelo Forteza S, De Cat P, Derekas A, Kayhan C, Ozuyar D, Skarka M, Hey DR, Shi F, Bowman DM, Kobzar O, Ayala Gomez A, Bognar Zs, Buzasi DL, Ebadi M, Fox-Machado L, Garcia Hernandez A, Ghasemi H, Guzik JA, Handberg R, Handler G, Hasanzadeh A, Jayaraman R, Khalack V, Kochukhov O, Lovekin CC, Mikolajczyk P, Mkrtichian D, Murphy SJ, Niemczura E, Olafsson BG, Pascual-Granado J, Paunzen E, Posilek N, Ramon-Ballesta A, Safari H, Samadi-Ghadim A, Smalley B, Sodor A, Stateva I, Suarez JC, Szabo R, Wu T, Ziaali E, Zong W, Seager S

Publication type: Article

Publication status: Published

Journal: Monthly Notices of the Royal Astronomical Society

Year: 2024

Volume: 527

Issue: 4

Pages: 9548-9580

Print publication date: 01/01/2024

Online publication date: 08/12/2023

Acceptance date: 07/12/2023

Date deposited: 23/01/2024

ISSN (print): 0035-8711

ISSN (electronic): 1365-2966

Publisher: Oxford University Press

URL: https://doi.org/10.1093/mnras/stad3800

DOI: 10.1093/mnras/stad3800


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Funding

Funder referenceFunder name
Fundação para a Ciência e Tecnologia FCT/MCTES, Portugal UIDB/04434/2020, UIDP/04434/2020.FCT, 2022.03993.PTDC and CEECIND/02619/2017
KKP-137523 ‘SeismoLab’ Èlvonal grant of the Hungarian Research, Development and Innovation Office (NKFIH)
NASA (NNX16AB76G, 80NSSC22K0622
Research Foundation Flanders 1286521N
PAPIIT IN117323
Spanish public funds ESP2017-87676-C5-5-R
the B-type Strategic Priority Program of Chinese Academy of Sciences (grant no. XDB41000000)
the Hungarian Research, Development and Innovation Office (NKFIH)
Programas Estatales de Generación de Conocimiento y Fortalecimiento Científico y Tecnológico del Sistema de I + D + i y de I + D + i Orientada a los Retos de la Sociedad PID2019-107061GB-C63
the MW-Gaia COST Action (CA18104)
the National Natural Science Foundation of China (NSFC) no. 12273002 and 12090040/2
the National Natural Science Foundation of China 2133011 and 12273104
the Natural Sciences and Engineering Research Council of Canada (NSERC)
the Spanish State Research Agency (AEI) Projects No. PID2019-107061GB-C64
the Whitaker Endowed Fund at Florida Gulf Coast University
the Youth Innovation Promotion Association of Chinese Academy of Sciences
the Yunnan Ten Thousand Talents Plan Young & Elite Talents Project, and from the International Centre of Supernovae, Yunnan Key Laboratory (No. 202302AN360001)
the ELTE Eötvös Loránd University and the European Space Agency (ESA-D/SCI-LE-2021-0025)
the National Key Research and Development Program of China (grant no. 2021YFA1600402)
the Polish National Science Center (NCN) 2021/43/B/ST9/02972
the Science and Technology Facilities Council (STFC) ST/M000877/1
the Severo Ochoa grant CEX2021-001131-S MCIN/AEI/10.13039/501100011033
the UK government’s Horizon Europe funding guarantee EP/Y031059/1
VILLUM FONDEN 00028173

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