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Implication of the period-magnitude relation for massive AGB stars and its astronomical applications

Published online by Cambridge University Press:  06 February 2024

Akiharu Nakagawa Open the ORCID record for Akiharu Nakagawa [Opens in a new window] ,
Tomoharu Kurayama ,
Hiroshi Sudou  and
Gabor Orosz Open the ORCID record for Gabor Orosz [Opens in a new window]
Akiharu Nakagawa*
Affiliation:
Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065, Japan
Tomoharu Kurayama
Affiliation:
Teikyo University of Science, 2-2-1 Senju-Sakuragi, Adachi-ku, Tokyo 120-0045, Japan
Hiroshi Sudou
Affiliation:
Department of General Engineering, National Institute of Technology, Sendai College, Natori Campus, 48 Nodayama, Medeshima-Shiote, Natori-shi, Miyagi 981-1239, Japan
Gabor Orosz
Affiliation:
Joint Institute for VLBI ERIC (JIVE), Oude Hoogeveensedijk 4, 7991 PD, Dwingeloo, Netherlands
*
email: [email protected]
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Abstract

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We present astrometric very long baseline interferometry (VLBI) studies of AGB stars. To understand the properties and evolution of AGB stars, distances are an important parameter. The distribution and kinematics of their circumstellar matter are also revealed with the VLBI method. We used the VERA array to observe 22 GHz H2O masers in various subclasses of AGB stars. Parallaxes of the three OH/IR stars NSV17351, OH39.7+1.5, IRC−30363, and the Mira-type variable star AW Tau were newly obtained. We present the circumstellar distribution and kinematics of H2O masers around NSV17351. The absolute magnitudes in mid-infrared bands of OH/IR stars with very long pulsation periods were investigated and a period-magnitude relation in the WISE W3 band, MW3 = (−7.21 ± 1.18) log P + (9.25 ± 3.09), was found for the Galactic AGB stars. The VLBI is still a powerful tool for parallax measurements of the Galactic AGB stars surrounded by thick dust shells.

Keywords

VLBIAstrometryMasersAGB starsOH/IR stars
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S376: At the crossroads of astrophysics and cosmology: Period–luminosity relations in the 2020s , December 2022 , pp. 159 - 179
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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