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Covariations of chromospheric and photometric variability of the young Sun analogue HD 30495: evidence for and interpretation of mid-term periodicities
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Document Type
Version of Record
Authors
W Soon (Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, 02138, USA)
V M Velasco Herrera (Instituto de Geofísica, Universidad Nacional Autónoma de México, Circuito Exterior, C. U., Coyoacán, CDMX, 04510, México)
R G Cionco (Comisión de Investigaciones Científicas (CIC), Provincia de Buenos Aires - Universidad Tecnológica Nacional (UTN), Colón 332, San Nicolás, Buenos Aires, Argentina)
S Qiu (Department of Geophysics, College of the Geology Engineering and Geomatics, Chang’an University, Xi’an, 710064, China; and Key Laboratory of Geospace Environment, Chinese Academy of Sciences, University of Science and Technology of China, Hefei, 230026, China)
S Baliunas (Retired, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA)
R Egeland (High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80307-3000, USA)
G W Henry (Center of Excellence in Information Systems, Tennessee State University, Nashville, TN 37209, USA)
I Charvátová (Institute of Geophysics, Academy of Sciences, Praha 4, 141 31, Czech Republic)
Date Acquired
February 10, 2024
Publication Date
December 3, 2018
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 483
Issue: 2
Issue Publication Date: February 21, 2019
ISSN: 0035-8711
e-ISSN: 1365-2966
DOI: 10.1093/mnras/sty3290
Distribution Limits
Public
Keywords
space and planetary science
astronomy and astrophysics

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