pith. sign in

arxiv: astro-ph/0411564 · v1 · pith:3EI35D4Jnew · submitted 2004-11-19 · 🌌 astro-ph

A general catalogue of 6.7 GHz methanol masers. I: data

classification 🌌 astro-ph
keywords masersmethanolcatalogueobjectsassociatedfurthergalacticregions
0
0 comments X
read the original abstract

Methanol masers are often detected in regions of intense star formation. Several studies in the last decade indicate that they may even be the earliest signpost of a high-mass star-forming region. Their powerful emission make them very good candidates for observations using both single--dish telescopes and interferometers, the latter allows detailed structural and dynamical studies of these objects. We have prepared a catalogue of all known 6.7-GHz methanol masers, discovered both by surveys that targeted possible associated objects and unbiased surveys covering a large fraction of galactic longitudes across the Galactic plane (-0.5deg <= b <= 0.5deg for most of the regions). The catalogue contains 519 sources which are listed with their kinematic (galactocentric and heliocentric) distances as well as possibly associated IR objects. We find that 6.7-GHz methanol masers clearly trace the molecular ring of our Galaxy, where most of the OB associations are located. The present list of masers also reports detections of other masing transitions of methanol as further information for the study of the maser phenomenon. In a further publication we will address some statistical considerations.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Star Formation at the Periphery of a Molecular Superbubble: The Case of G12.79+0.43

    astro-ph.GA 2026-06 unverdicted novelty 3.0

    Observational study of G12.79+0.43 identifies YSOs and HII regions powered by B-type stars and associates the complex with the rim of a molecular superbubble of diameter ~50 pc and expansion age ~0.3 Myr without estab...

  2. Polarization Observations of a Sample of 6.7 GHz Methanol Masers

    astro-ph.GA 2026-05 unverdicted novelty 3.0

    Polarization observations of 6.7 GHz methanol masers show linear and circular components with Zeeman splitting that varies over time, interpreted as evidence for changing magnetic fields.

  3. Cosmic Rulers: Masers as Tools for Probing Structure in the Galaxy and Beyond, from AU to kpc

    astro-ph.GA 2026-06 unverdicted novelty 2.0

    Maser emissions act as cosmic rulers for astrometric measurements of astronomical sources from protostellar scales to galactic distances, with SKA-Mid enabling expanded multi-species observations.