M2P2 I:玛泽监测帕克斯计划数据说明和斯托克斯-I OH 玛泽变异性

IF 4.5 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Publications of the Astronomical Society of Australia Pub Date : 2024-01-25 DOI:10.1017/pasa.2024.3
Anita Hafner, James A. Green, Ashie Burdon, Elena Popova, Dmitry Ladeyschikov, Shari Breen, Ross Alexander Burns, James O. Chibueze, M. D. Gray, Busaba Hutawarakorn Kramer, Gordon MacLeod, Andrey Sobolev, Maxim Voronkov
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引用次数: 0

摘要

Maser监测帕克斯项目(M2P2)是一个正在进行的项目,旨在利用位于墨里昂的64米CSIRO帕克斯射电望远镜观测高质量恒星形成区(HMSFR)的maser。在本文中,我们将概述该项目,并介绍前两年观测到的斯托克斯-I数据。在该项目观测的 63 条视线中,我们总共识别出 1514 个单独的 maser 特征:其中 14.4%(203 个)的 27 条观测线显示出显著的变异性。其中大部分(160/203)出现在 1665 和 1667MHz 的 OH 主线跃迁中,但该数据集还包括 1612 和 1720MHz 卫星线上的大量可变特征(分别为 33 和 10),其中大部分(分别为 24 和 9)似乎与 HMSFRs 有关。根据其强度随时间的变化,我们将这些特征分为四大类:耀斑(6%)、周期性(11%)、长期趋势(33%)和 "其他"(50%)。可变 masers 为模拟 HMSFRs 的局部环境条件提供了一个独特的实验室,后续出版物将对此进行更详细的研究。
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M2P2 I: Maser Monitoring Parkes Program data description and Stokes-I OH maser variability
The Maser Monitoring Parkes Project (M2P2) is an ongoing project to observe masers towards high mass star forming regions (HMSFRs) using the 64m CSIRO Parkes radio telescope, Murriyang. In this paper we outline the project and introduce Stokes-I data from the first two years of observations. For the 63 sightlines observed in this project we identify a total of 1514 individual maser features: 14.4% of these (203) towards 27 sightlines show significant variability. Most of these (160/203) are seen in the main-line transitions of OH at 1665 and 1667 MHz, but this data set also includes a significant number of variable features in the satellite lines at 1612 and 1720MHz (33 and 10 respectively), most of which (24 and 9 respectively) appear to be associated with the HMSFRs. We divide these features into 4 broad categories based on the behaviour of their intensity over time: flares (6%), periodic (11%), long-term trends (33%) and ‘other’ (50%). Variable masers provide a unique laboratory for the modelling of local environmental conditions of HMSFRs, and follow-up publications will delve into this in more detail.
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来源期刊
Publications of the Astronomical Society of Australia
Publications of the Astronomical Society of Australia 地学天文-天文与天体物理
CiteScore
5.90
自引率
9.50%
发文量
41
审稿时长
>12 weeks
期刊介绍: Publications of the Astronomical Society of Australia (PASA) publishes new and significant research in astronomy and astrophysics. PASA covers a wide range of topics within astronomy, including multi-wavelength observations, theoretical modelling, computational astronomy and visualisation. PASA also maintains its heritage of publishing results on southern hemisphere astronomy and on astronomy with Australian facilities. PASA publishes research papers, review papers and special series on topical issues, making use of expert international reviewers and an experienced Editorial Board. As an electronic-only journal, PASA publishes paper by paper, ensuring a rapid publication rate. There are no page charges. PASA''s Editorial Board approve a certain number of papers per year to be published Open Access without a publication fee.
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