Ground-state OH maser distributions in the Galactic Centre region

Hai Hua Qiao; Andrew J. Walsh; Zhi Qiang Shen; Joanne R. Dawson

doi:10.1017/S1743921316011765

Ground-state OH maser distributions in the Galactic Centre region

Hai Hua Qiao, Andrew J. Walsh, Zhi Qiang Shen, Joanne R. Dawson

Research output: Contribution to journal › Conference paper › peer-review

Abstract

Ground-state OH masers identified in the Southern Parkes Large-Area Survey in Hydroxyl were observed with the Australia Telescope Compact Array to obtain positions with high accuracy (∼1 arcsec). We classified these OH masers into evolved star OH maser sites, star formation OH maser sites, supernova remnant OH maser sites, planetary nebula OH maser sites and unknown maser sites using their accurate positions. Evolved star and star formation OH maser sites in the Galactic Centre region (between Galactic longitudes of -5° to +5° and Galactic latitudes of -2° and +2°) were studied in detail to understand their distributions.

Original language	English
Pages (from-to)	141-142
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	11
Issue number	S322
DOIs	https://doi.org/10.1017/S1743921316011765
Publication status	Published - 2016
Event	International Astronomical Union Symposia 322 - Cairns, Australia Duration: 18 Jul 2016 → 22 Jul 2016 https://www.iau.org/science/meetings/past/symposia/1155/

Keywords

Galaxy: center
masers
stars: AGB and post-AGB
stars: formation

Access to Document

10.1017/S1743921316011765

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title = "Ground-state OH maser distributions in the Galactic Centre region",

abstract = "Ground-state OH masers identified in the Southern Parkes Large-Area Survey in Hydroxyl were observed with the Australia Telescope Compact Array to obtain positions with high accuracy (∼1 arcsec). We classified these OH masers into evolved star OH maser sites, star formation OH maser sites, supernova remnant OH maser sites, planetary nebula OH maser sites and unknown maser sites using their accurate positions. Evolved star and star formation OH maser sites in the Galactic Centre region (between Galactic longitudes of -5° to +5° and Galactic latitudes of -2° and +2°) were studied in detail to understand their distributions.",

keywords = "Galaxy: center, masers, stars: AGB and post-AGB, stars: formation",

author = "Qiao, {Hai Hua} and Walsh, {Andrew J.} and Shen, {Zhi Qiang} and Dawson, {Joanne R.}",

year = "2016",

doi = "10.1017/S1743921316011765",

language = "English",

volume = "11",

pages = "141--142",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

number = "S322",

note = "International Astronomical Union Symposia 322, IAUS 322 ; Conference date: 18-07-2016 Through 22-07-2016",

url = "https://www.iau.org/science/meetings/past/symposia/1155/",

}

TY - JOUR

T1 - Ground-state OH maser distributions in the Galactic Centre region

AU - Qiao, Hai Hua

AU - Walsh, Andrew J.

AU - Shen, Zhi Qiang

AU - Dawson, Joanne R.

PY - 2016

Y1 - 2016

N2 - Ground-state OH masers identified in the Southern Parkes Large-Area Survey in Hydroxyl were observed with the Australia Telescope Compact Array to obtain positions with high accuracy (∼1 arcsec). We classified these OH masers into evolved star OH maser sites, star formation OH maser sites, supernova remnant OH maser sites, planetary nebula OH maser sites and unknown maser sites using their accurate positions. Evolved star and star formation OH maser sites in the Galactic Centre region (between Galactic longitudes of -5° to +5° and Galactic latitudes of -2° and +2°) were studied in detail to understand their distributions.

AB - Ground-state OH masers identified in the Southern Parkes Large-Area Survey in Hydroxyl were observed with the Australia Telescope Compact Array to obtain positions with high accuracy (∼1 arcsec). We classified these OH masers into evolved star OH maser sites, star formation OH maser sites, supernova remnant OH maser sites, planetary nebula OH maser sites and unknown maser sites using their accurate positions. Evolved star and star formation OH maser sites in the Galactic Centre region (between Galactic longitudes of -5° to +5° and Galactic latitudes of -2° and +2°) were studied in detail to understand their distributions.

KW - Galaxy: center

KW - masers

KW - stars: AGB and post-AGB

KW - stars: formation

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U2 - 10.1017/S1743921316011765

DO - 10.1017/S1743921316011765

M3 - Conference paper

AN - SCOPUS:85012262935

VL - 11

SP - 141

EP - 142

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S322

T2 - International Astronomical Union Symposia 322

Y2 - 18 July 2016 through 22 July 2016

ER -