A Catalog of CH3OH 70-61 A+ Maser Sources in Massive Star-forming Regions

By S. Kurtz, P. Hofner, C. Álvarez. 2004

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ON THE NATURE OF THE LOCAL SPIRAL ARM OF THE MILKY WAY (2013, background): “Individual Sources ON 1 is associated with IRAS 20081+3122, which coincides with an ultra-compact HII (UC HII) region (Kurtz et al. 2004).”
Hierarchical fragmentation and differential star formation in the Galactic ‘Snake’: infrared dark cloud G11.11−0.12 (2014, background): “In this scenario, M1 traces the red lobe of the outflow (De Buizer 2003; Kurtz et al. 2004),but its velocity range spans blue to red (22–34 km s−1; § 4.2), and it becomes difficult to explain the ordered velocity field of M1 that could otherwise perfectly trace a disc (Pillai et al. 2006b).”
A CLASS I AND CLASS II CH3OH MASER SURVEY OF EGOs FROM THE GLIMPSE SURVEY (2009, background): “Only ∼29% of the masers reported by Kurtz et al. (2004) have peak flux densities – 4 –”
A study of the Keplerian accretion disk and precessing outflow in the massive protostar IRAS 20126+4104 (2005, unknown): “It is interesting to note that Kurtz et al. (2004) have detected several CH3OH maser spots at 44 GHz lying along the border of the thermal CH3OH emission in the jet, as shown in the upper panel of Fig.”
TADPOL: A 1.3 mm SURVEY OF DUST POLARIZATION IN STAR-FORMING CORES AND REGIONS (2013, background): “DR21(OH) is rich in methanol, water and OH maser features (Plambeck & Menten 1990; Liechti & Walmsley 1997; Kurtz et al. 2004; Araya et al. 2009).”