A survey of the 6.7 GHz methanol maser emission from IRAS sources - I. Data
By M. Szymczak, G. Hrynek, A. Kus. 2000
169 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Spectroscopy
View Paper: https://www.semanticscholar.org/paper/48c26f1426b6df8d92fab7f852c58f36e3688920
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In Astronomy and Astrophysics
- S. Ellingsen
- D. Ward-Thompson
- V. Minier
- E. Churchwell
- C. Cyganowski
- Michele Pestalozzi
- R. Booth
- A. Walsh
In Spectroscopy
Citations in the corpus
- A general catalogue of 6.7-GHz methanol masers. I. Data. (2004, methodology): “The surveys were conducted by MacLeod et al. (1992); MacLeod & Gaylard (1992); Gaylard & MacLeod (1993); Schutte et al. (1993); Caswell et al. (1995); Van der Walt et al. (1995, 1996); Walsh et al. (1997); Slysh et al. (1999); Szymczak et al. (2000a).”
- The 6-GHz methanol multibeam maser catalogue – II. Galactic longitudes 6° to 20° (2010, background): “16.864- 2.159 was originally discovered by Caswell et al. (1995a) in a targeted search towards OH masers and has since been observed by Walsh et al. (1997, 1998) and Szymczak et al. (2000).”
- A CLASS I AND CLASS II CH3OH MASER SURVEY OF EGOs FROM THE GLIMPSE SURVEY (2009, background): “The velocity coverage of our observations does not extend to the H 2 O maser velocities (∼66-70 km s −1 ), but neither Szymczak et al. (2000) nor Pandian et al. (2007) report 6.7 GHz CH 3 OH maser emission outside the range of ∼40-47 km s −1 in their much wider bandwidth single-dish spectra.”
- Methanol Masers: Reliable Tracers of the Early Stages of High-Mass Star Formation (2005, background): “Many methanol masers have been discovered in searches towards IRAS sources which meet the Wood & Churchwell (1989) criteria for being ultra-compact Hii regions (e.g. Schutte et al. 1993; van der Walt et al. 1995; Walsh et al. 1997; Slysh et al. 1999; Szymczak et al. 2000).”
- The 6-GHz multibeam maser survey-I. Techniques (2008, background): “…sites), other targeted methanol maser searches have produced detection rates of about 15 per cent (MacLeod et al. 1992; MacLeod & Gaylard 1992; Gaylard & MacLeod 1993; Schutte et al. 1993; van der Walt et al. 1995, 1996; Walsh et al. 1997; Slysh et al. 1999; Szymczak et al. 2000; Ellingsen 2007).”