Probing the early phases of high mass star formation with 6.7 GHz methanol masers
arXiv:1912.06973 · doi:10.1093/mnras/stz3558
Abstract
Methanol masers at 6.7 GHz are the brightest of class II methanol masers and have been found exclusively towards massive star forming regions. These masers can thus be used as a unique tool to probe the early phases of massive star formation. We present here a study of the spectral energy distributions of 320 6.7 GHz methanol masers chosen from the MMB catalogue, which fall in the Hi-GAL range (, ). The spectral energy distributions are constructed from m using data from the ATLASGAL and Hi-GAL surveys. The emission from cold dust is modelled by a single grey body component fit. We estimate the clump properties such as mass, FIR luminosity and column density using the best fit parameters of the SED fits. Considering the Kauffman criteria for massive star formation, we find that all but a few maser hosts have the potential to harbour at least one high mass star. The physical properties of the methanol maser hosts are also discussed. The evolutionary stages of 6.7 GHz maser sources, explored using the mass luminosity diagram, suggests that they are predominantly associated with high mass stars with the majority being in the accretion phase. However, we observe a small number of sources that could possibly be related to intermediate or low-mass stars.
arXiv comment15 pages, 13 figures, accepted for publication in MNRAS
References in corpus (41)
- On the variation of the Initial Mass Function
- Embedded Clusters in Molecular Clouds
- Trigonometric Parallaxes of High Mass Star Forming Regions: the Structure and Kinematics of the Milky Way
- GLIMPSE: I. A SIRTF Legacy Project to Map the Inner Galaxy
- Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
- The Formation of Massive Stars from Turbulent Cores
- Cold Dark Clouds: The Initial Conditions for Star Formation
- Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting observed SEDs using a large grid of pre-computed models
- ATLASGAL - The APEX Telescope Large Area Survey of the Galaxy at 870 microns
- Hi-GAL: the Herschel infrared Galactic Plane Survey
- Competitive accretion in embedded stellar cluster
- A Parallax-based Distance Estimator for Spiral Arm Sources
- ATLASGAL - Compact source catalogue: 330 < l < 21 degrees
- The 6-GHz methanol multibeam maser catalogue I: Galactic Centre region, longitudes 345 to 6
- Ammonia in Infrared Dark Clouds
- The Bolocam Galactic Plane Survey -- II. Catalog of the Image Data
- ATLASGAL --- towards a complete sample of massive star forming clumps
- The ATLASGAL survey: a catalog of dust condensations in the Galactic plane
- The uncertainty in Galactic parameters
- Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ()
- Methanol masers : Reliable tracers of the early stages of high-mass star formation
- From Massive Protostars to a Giant HII Region: Submillimeter Imaging of the Galactic Mini-starburst W43
- Characterizing Precursors to Stellar Clusters with Herschel
- ATLASGAL --- Environments of 6.7\,GHz methanol masers
- The Mass-Size Relation from Clouds to Cores. II. Solar Neighborhood Clouds
- Confirmation of the exclusive association between 6.7-GHz methanol masers and high-mass star formation regions
- A high-sensitivity 6.7 GHz methanol maser survey toward H2O sources
- The Mass-Size Relation from Clouds to Cores. I. A new Probe of Structure in Molecular Clouds
- Simultaneous low- and high-mass star formation in a massive protocluster: ALMA observations of G11.92-0.61
- Dust in the diffuse emission of the galactic plane - The Herschel/Spitzer SED fitting
- The almost ubiquitous association of 6.7 GHz methanol masers with dust
- The Arecibo Methanol Maser Galactic Plane Survey - III: Distances and Luminosities
- Triggered/sequential star formation? A multi-phase ISM study around the prominent IRDC G18.93-0.03
- 6.7GHz Methanol Maser Associated Outflows: An evolutionary sequence
- On the Identification of High Mass Star Forming Regions using IRAS: Contamination by Low-Mass Protostars
- Hyper: Hybrid Photometry and Extraction Routine
- Detection of 6.7 GHz methanol absorption towards hot corinos
- How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps?
- Spectral Energy Distributions of 6.7 GHz methanol masers
- Physical conditions around 6.7 GHz methanol masers-I: Ammonia
- Radio Observations of the Star Formation Activities in the NGC 2024 FIR 4 Region
Cited by in corpus (6)
- A Global View on Star Formation: The GLOSTAR Galactic Plane Survey V. 6.7 GHz Methanol Maser Catalogue
- Upper Mass-Loss Limits and Clumping in the Intermediate and Outer Wind Regions of OB stars
- A global view on star formation: The GLOSTAR Galactic plane survey III. 6.7 GHz methanol maser survey in Cygnus X
- A global view on star formation: The GLOSTAR Galactic plane survey X. Galactic HII region catalog using radio recombination lines
- Radio and infrared study of the supernova remnant candidate HESS J1912+101
- Chemical environments of 6.7 GHz methanol maser sources