2000
DOI: 10.1086/309165
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Kinematics and Distance of Water Masers in W3 IRS 5

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Cited by 91 publications
(122 citation statements)
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“…W3 IRS5 is a massive star-forming region located in the Perseus arm at a distance of 1.83 ± 0.14 kpc (Imai et al 2000) with a total luminosity of 2 × 10 5 L (Campbell et al 1995). A cluster of hypercompact (<240 AU) H II regions are found from high-resolution cm-wavelength observations (Claussen et al 1994;Wilson et al 2003;van der Tak et al 2005).…”
Section: Introductionmentioning
confidence: 99%
“…W3 IRS5 is a massive star-forming region located in the Perseus arm at a distance of 1.83 ± 0.14 kpc (Imai et al 2000) with a total luminosity of 2 × 10 5 L (Campbell et al 1995). A cluster of hypercompact (<240 AU) H II regions are found from high-resolution cm-wavelength observations (Claussen et al 1994;Wilson et al 2003;van der Tak et al 2005).…”
Section: Introductionmentioning
confidence: 99%
“…Based on these predictions, the "Radiation Diagnostics" observations started with deep integrations of a large number of hydrides that was to be followed by a survey of a few species in many sources of various ages and masses. Here we present exploratory observations towards W3 IRS5, a nearby region (1.83 kpc, Imai et al 2000) of high-mass star formation, moving at -38.4 km s −1 in the local standard of rest (LSR). W3 IRS5 resembles the Trapezium cluster in Orion but is considerably younger.…”
Section: Introductionmentioning
confidence: 99%
“…The W3 giant molecular cloud (GMC) complex is located in the Perseus spiral arm at a distance of 1:83 AE 0:14 kpc from the Sun (Imai et al 2000). The W3 GMC hosts two massive and active star-forming regions, W3 Main in the north and W3(OH) in the south.…”
Section: Introductionmentioning
confidence: 99%