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The power of heartbeats through the lens of ι Orionis

Pablo, H. and Richardson, N. D. and Fuller, J. and Moffatt, A. F. J. (2017) The power of heartbeats through the lens of ι Orionis. In: Second BRITE-Constellation Science Conference - Small satellites - big science. Proceedings of the Polish Astronomical Society. No.5. Polish Astronomical Society , Warsaw, Poland, pp. 167-172. ISBN 978-83-938279-6-1. https://resolver.caltech.edu/CaltechAUTHORS:20190426-104557821

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Abstract

O star asteroseismology is a relatively new field which has not been able to gain significant traction due in large part to the lack of known pulsators in addition to the relatively sparse number of frequencies detected in those pulsators. This is likely due to a combination of factors, chief among them long frequencies, on the order of days, and weak amplitudes (≈ 1 mmag and below). Fortunately, through the discovery of the most massive heartbeat system ι Orionis and it's corresponding tidally induced oscillations with BRITE-Constellation there exists a new avenue with which to explore O star asteroseismology. In this paper we will give a prescription for using tidally induced oscillations to do asteroseismic analysis on O stars and present a list of candidate systems for this analysis within the BRITE sample.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://www.pta.edu.pl/proc/v5p167PublisherArticle
ORCID:
AuthorORCID
Pablo, H.0000-0002-1355-5860
Richardson, N. D.0000-0002-2806-9339
Fuller, J.0000-0002-4544-0750
Additional Information:© 2016 Polskie Towarzystwo Astronomiczne. Based on data collected by the BRITE Constellation satellite mission, designed, built, launched, operated and supported by the Austrian Research Promotion Agency (FFG), the University of Vienna, the Technical University of Graz, the Canadian Space Agency (CSA), the University of Toronto Institute for Aerospace Studies (UTIAS), the Foundation for Polish Science & Technology (FNiTP MNiSW), and National Science Centre (NCN). NDR acknowledges postdoctoral support by the University of Toledo and by the Helen Luedtke Brooks Endowed Professorship. AFJM is grateful for financial aid from NSERC (Canada) and FQRNT (Quebec).
Group:TAPIR, Walter Burke Institute for Theoretical Physics, Astronomy Department
Funders:
Funding AgencyGrant Number
Österreichische Forschungsförderungsgesellschaft (FFG)UNSPECIFIED
University of ViennaUNSPECIFIED
Technical University of GrazUNSPECIFIED
Canadian Space Agency (CSA)UNSPECIFIED
University of TorontoUNSPECIFIED
Foundation for Polish Science & Technology (FNiTP MNiSW)UNSPECIFIED
National Science Centre (Poland)UNSPECIFIED
University of ToledoUNSPECIFIED
Helen Luedtke Brooks Endowed ProfessorshipUNSPECIFIED
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
Fonds de recherche du Québec-Nature et technologies (FRQ-NT)UNSPECIFIED
Series Name:Proceedings of the Polish Astronomical Society
Issue or Number:5
Record Number:CaltechAUTHORS:20190426-104557821
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190426-104557821
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95023
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:26 Apr 2019 18:13
Last Modified:09 Mar 2020 13:19

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