Water Masers Toward Ultracompact HII Regions
arXiv:astro-ph/0507039 · doi:10.1086/431546
Abstract
We present a survey in the 6_{16}-5_{23} rotational water transition toward 33 galactic ultracompact HII regions. Maser emission is detected toward 18 of these sources; two are new detections. High quality spectra are provided for all 18 sources. We discuss the detection rate of this survey and the correlation of various maser properties with other physical parameters. In addition, we report wide-bandwidth (316 km/s), moderate-resolution (~ 3'') water maser observations of the HH80-81 region. We report the first detection of water maser emission at the approximate velocity of the molecular core. This emission is coincident with the extreme tip of the thermal jet, and well-removed from the much stronger and well-known maser emission at the position of VLA-3.
arXiv comment21 pages, 5 figures. Accepted by Astronomical Journal
References in corpus (7)
- Massive Stars: Their Environment and Formation
- CH3OH and H2O masers in high-mass star-forming regions
- Long-term study of water masers associated with Young Stellar Objects. II: Analysis
- A survey for water maser emission towards planetary nebulae. New detection in IRAS 17347-3139
- VLA and BIMA observations toward the exciting source of the massive HH~80-81 outflow
- The structure of Onsala 1 star forming region
- Water masers in dusty environments
Cited by in corpus (32)
- The RMS Survey: Ammonia and water maser analysis of massive star forming regions
- A near IR imaging survey of intermediate and high-mass young stellar outflow candidates
- ATOMS:ALMA Three-millimeter Observations of Massive Star-forming regions -- III :Catalogues of candidate hot molecular cores and Hyper/Ultra compact HII regions
- The RMS Survey: H2O masers towards a sample of southern hemisphere massive YSO candidates and ultra compact HII regions
- GLOSTAR -- Radio Source Catalog I: and
- A Multi-Epoch, Simultaneous Water and Methanol Maser Survey toward Intermediate-Mass Young Stellar Objects
- A population of hypercompact HII regions identified from young HII regions
- ATLASGAL-selected massive clumps in the inner Galaxy IV. Millimeter hydrogen recombination lines from associated HII regions
- Astrometry of Galactic Star-Forming Region G48.61+0.02 with VERA
- Molecular outflows around high-mass young stellar objects
- Millimeter and submillimeter high angular resolution interferometric observations: dust in the heart of IRAS 18162-2048
- A multiwavelength study of star formation in the vicinity of Galactic HII region Sh2-100
- A VLA Study of Ultracompact and Hypercompact H II Regions from 0.7 to 3.6 cm
- The G305 star-forming complex: radio continuum and molecular line observations
- Water Masers Associated with Star Formation in the Antennae Galaxies
- Ionized Gas Towards Molecular Clumps: Physical Properties of Massive Star Forming Regions
- Identification of Very Red Counterparts of SiO Maser and OH/IR Objects in the GLIMPSE Survey
- Unveiling a cluster of protostellar disks around the massive protostar GGD27 MM1
- VLBI Observations of Water Masers in Onsala 1: Massive Binary Star Forming Site?
- Superflares of HO Maser Emission in the Protostellar Object IRAS 183160602
- Surveys of Clumps, Cores, and Condensations in the Cygnus X: II. Radio Properties of the Massive Dense Cores
- SCOTCH -- Search for Clandestine Optically Thick Compact HIIs
- Water Masers in the Andromeda Galaxy: I. A Survey for Water Masers, Ammonia, and Hydrogen Recombination Lines
- Study of the dense molecular gas surrounding the "Extended Green Object" G35.03+0.35
- A gallery of bubbles - The nature of the bubbles observed by Spitzer and what ATLASGAL tells us about the surrounding neutral material
- SCOTCH Search for Clandestine Optically Thick Compact HII regions II
- Water Masers in the Andromeda Galaxy: II. Where Do Masers Arise?
- A Possible Chemical Clock in High-mass Star-forming Regions: N(HC3N)/N(N2H+)?
- Erosion of a dense molecular core by a strong outflow from a massive protostar
- A Molecular Line Investigation of the Interaction between Mid-infrared Bubbles and the Interstellar Medium
- The SOFIA Massive (SOMA) Star Formation Q-band Follow-up. II. Hydrogen Recombination Lines Toward High-Mass Protostars
- Simultaneous 22 GHz Water and 44 GHz Methanol Masers Survey of Ultracompact HII Regions