The 6-GHz methanol multibeam maser catalogue – I. Galactic Centre region, longitudes 345° to 6°

By J. Caswell, G. Fuller, J. Green, A. Avison, S. Breen, K. Brooks, M. Burton, A. Chrysostomou, J. Cox, P. Diamond and 15 more. 2010

223 citations recorded by the source corpus.

Original article can be found at: http://www3.interscience.wiley.com/journal/ Copyright Royal Astronomical Society

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/2329a5e8481084dc0475d9d540ba86a4cf726642

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Citations in the corpus

• Molecular gas kinematics within the central 250 pc of the Milky Way (2016, background): “253+0.016, and in the dust ridge clouds C and E (e.g. Caswell et al. 2010; Walsh et al. 2014; Lu et al., in prep.).”
• The Bar and Spiral Structure Legacy (BeSSeL) Survey: Mapping the Milky Way with VLBI Astrometry† (2011, background): “…6.7 GHz methanol masers by Pestalozzi et al. (2005) lists more than 500 sources, and many more were found recently with Arecibo (Pandian et al. 2007), Effelsberg (Xu et al. 2008), and in particular in the methanol multi beam survey on the Parkes telescope (Caswell et al. 2010; Green et al. 2010).”
• THE RED MSX SOURCE SURVEY: THE MASSIVE YOUNG STELLAR POPULATION OF OUR GALAXY (2013, background): “Caswell et al. 2010, Contreras et al. 2013, Molinari et al. 2010), a complete census, and understanding of the evolution, of the massive star population from initial core through to main sequence will be possible.”
• Variations in the Galactic star formation rate and density thresholds for star formation (2012, methodology): “Water masers are detected towards evolved stars, but these are found outside the diskplane and the emission is typically two orders of magnitude weaker (Caswell et al. 2010).”
• The 6-GHz methanol multibeam maser catalogue – II. Galactic longitudes 6° to 20° (2010, methodology): “Four are previously known and have been associated with the Galactic bar (see Caswell et al. 2010 for details).”
• Ammonia from cold high-mass clumps discovered in the inner Galactic disk by the ATLASGAL survey (2012, background): “…of young stellar objects (YSOs as dotted black curve) from the RMS survey (Hoare et al. 2005), CH3OH masers from Pandian et al. (2011), Szymczak et al. (2002), and Caswell et al. (2010) (dashed and dashed-dotted curves) and the ATLASGAL sample as a solid curve in green in the middle panel.”
• ATLASGAL — towards a complete sample of massive star forming clumps ⋆ (2014, background): “…Survey of the Galaxy (ATLASGAL), Schuller et al. 2009; Bolocam Galactic Plane Survey (BGPS), Aguirre et al. 2011; methanol multibeam (MMB) survey, Caswell et al. 2010; and the Co-ordinated Radio and Infrared Survey for High-Mass Star Formation (CORNISH), Hoare et al. 2012; Purcell et al. 2013).”
• THE GREEN BANK TELESCOPE H ii REGION DISCOVERY SURVEY. II. THE SOURCE CATALOG (2011, background): “Although these ten sources show that star formation is ongoing in the nuclear disk, Caswell et al. (2010) find no methanol masers with nuclear disk velocities.”
• The observed spiral structure of the Milky Way (2014, background): “The most important progress of the 6.7 GHz methanol maser discovery is the Methanol Multibeam (MMB) Survey of the entire Galactic plane (e.g., Green et al. 2009, 2010, 2012; Caswell et al. 2010, 2011).”