The 6-GHz methanol multibeam maser catalogue – II. Galactic longitudes 6° to 20°
By J. Green, J. Caswell, G. Fuller, A. Avison, S. Breen, S. Ellingsen, M. Gray, M. Pestalozzi, L. Quinn, M. Thompson and 1 more. 2010
132 citations recorded by the source corpus.
The definitive version is available at: http://onlinelibrary.wiley.com Copyright Royal Astronomical Society.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/6bb5099bbc6c730c9a34d7f7b6fefc488d425e28
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Citations in the corpus
- 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).”
- Variations in the Galactic star formation rate and density thresholds for star formation (2012, methodology): “We use data from HOPS and the methanol multibeam (MMB Caswell et al. 2010, 2011; Green et al. 2010, 2012) surveys to detect the 22 GHz water maser emission and 6.7 GHz Class II methanol maser emission, respectively, across the Galactic plane.”
- The observed spiral structure of the Milky Way (2014, background): “The 6.7 GHz methanol masers (Menten 1991) have been widely detected from massive star forming regions in our Galaxy (e.g., Pestalozzi et al. 2005; Ellingsen 2006; Green et al. 2010, 2012).”