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Tanabe Yoshihiro

Affiliate Master Yamaguchi University

Periodic 6.7 GHz CH_3OH Maser Emission in G353.273+0.641 : First Candidate for a Pulsating High-mass Protostar

The Astrophysical Journal Volume 997 Issue 2
published_at 2026-02-01
Harajiri_2026_ApJ_997_349.pdf
5.14 MB
Supplemental Data : https://public.oa.kenkyu.yamaguchi-u.ac.jp/cba5f7fa-4cce-444e-9e89-94f1b878b5f7
Title
Periodic 6.7 GHz CH_3OH Maser Emission in G353.273+0.641 : First Candidate for a Pulsating High-mass Protostar
Creators Harajiri Sohta
Creators Motogi Kazuhito
Affiliate Master Yamaguchi University
[kakenhi]15501 grid.268397.1
Creators Nakamura Ryota
Creators Yonekura Yoshinori
Creators Tanabe Yoshihiro
Affiliate Master Yamaguchi University
[kakenhi]15501 grid.268397.1
Creators Fujisawa Kenta
Affiliate Master Yamaguchi University
[kakenhi]15501 grid.268397.1
Source Identifiers [PISSN] 0004-637X [EISSN] 1538-4357
Languages eng
Resource Type journal article
Publishers American Astronomical Society
Date Issued 2026-02-01
Rights
© 2026. The Author(s). Published by the American Astronomical Society.()
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.()
Creative Commons Attribution 4.0 International(https://creativecommons.org/licenses/by/4.0/)
File Version Version of Record
Access Rights open access
Relations
[isIdenticalTo] 10.3847/1538-4357/ae30e3
[isSupplementedBy] [URI]https://public.oa.kenkyu.yamaguchi-u.ac.jp/cba5f7fa-4cce-444e-9e89-94f1b878b5f7
Funding Refs
Japan Society for the Promotion of Science [crossref_funder]https://doi.org/10.13039/501100001691
Award Observational study of the accretion burst--sudden flux rise of the methanol maser--associated with the intermittent accretion in the massive star formation 21H01120
Funding Refs
Japan Society for the Promotion of Science [crossref_funder]https://doi.org/10.13039/501100001691
Award メタノールメーザー高頻度観測による、大質量星形成時の質量降着率の時間変動の解明 21H00032