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 64 m 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 t...
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creator | Hafner, Anita Green, James A. Burdon, Ashie Popova, Elena Ladeyschikov, Dmitry Breen, Shari Burns, Ross Alexander Chibueze, James O. Gray, M. D. Kramer, Busaba Hutawarakorn MacLeod, Gordon Sobolev, Andrey Voronkov, Maxim |
description | The Maser Monitoring Parkes Project (M2P2) is an ongoing project to observe masers towards high-mass star-forming regions (HMSFRs) using the 64 m 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 1 514 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 1 612 and 1 720 MHz (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. |
doi_str_mv | 10.1017/pasa.2024.3 |
format | Article |
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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 1 612 and 1 720 MHz (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%). 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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 1 612 and 1 720 MHz (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%). 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D.</au><au>Kramer, Busaba Hutawarakorn</au><au>MacLeod, Gordon</au><au>Sobolev, Andrey</au><au>Voronkov, Maxim</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>M2P2 I: Maser Monitoring Parkes Program data description and Stokes-I OH maser variability</atitle><jtitle>Publications of the Astronomical Society of Australia</jtitle><addtitle>Publ. Astron. Soc. Aust</addtitle><date>2024-01-22</date><risdate>2024</risdate><volume>41</volume><artnum>e009</artnum><issn>1323-3580</issn><eissn>1448-6083</eissn><abstract>The Maser Monitoring Parkes Project (M2P2) is an ongoing project to observe masers towards high-mass star-forming regions (HMSFRs) using the 64 m 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 1 514 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 1 612 and 1 720 MHz (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%). 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title | M2P2 I: Maser Monitoring Parkes Program data description and Stokes-I OH maser variability |
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