1985
DOI: 10.1086/163573
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A wide-latitude CO survey of molecular clouds in the northern Milky Way

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Cited by 171 publications
(131 citation statements)
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“…Preliminary observations by Cohen & Thaddeus (1977) were expanded to a beamwidth-sampled survey of the plane by ; roughly the same area has recently been mapped in the CO (J \ 2È1) line with the same angular resolution and grid spacing by Sakamoto et al (1997). The Ðrst large-scale superbeam survey, with 1¡ angular resolution, was conducted in the Ðrst quadrant by Dame & Thaddeus (1985), and a subsequent survey at 0¡ .5 resolution was included in the composite survey of Dame et al (1987). The very sensitive observations included in the present composite map were begun in 1991 as a series of narrow, Nyquist-sampled strips perpendicular to the Galactic plane (survey 7) ; Dame & Thaddeus (1994) used this surveyÈwith the highest sensitivity per unit solid angle of any in the composite map (see col.…”
Section: First Quadrantmentioning
confidence: 99%
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“…Preliminary observations by Cohen & Thaddeus (1977) were expanded to a beamwidth-sampled survey of the plane by ; roughly the same area has recently been mapped in the CO (J \ 2È1) line with the same angular resolution and grid spacing by Sakamoto et al (1997). The Ðrst large-scale superbeam survey, with 1¡ angular resolution, was conducted in the Ðrst quadrant by Dame & Thaddeus (1985), and a subsequent survey at 0¡ .5 resolution was included in the composite survey of Dame et al (1987). The very sensitive observations included in the present composite map were begun in 1991 as a series of narrow, Nyquist-sampled strips perpendicular to the Galactic plane (survey 7) ; Dame & Thaddeus (1994) used this surveyÈwith the highest sensitivity per unit solid angle of any in the composite map (see col.…”
Section: First Quadrantmentioning
confidence: 99%
“…The 21 cm component corresponding to the clouds at [12 km s~1 was identiÐed with the Local spiral arm by Lindblad (1974) ; the other component, LindbladÏs feature A, was modeled by Lindblad et al (1973) and Grape (1975) as an expanding shell of cold gas surrounding the Sun and data with lower sensitivity and angular resolution is shown in Fig. 4 of Dame & Thaddeus (1985).…”
Section: Arge-scale Structurementioning
confidence: 99%
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“…Extensive surveys of the CO and 13 CO (J=1-0 at λ = 2.6 mm and J=2-1 at λ = 1.3 mm) emissions in the Galaxy have been used to determine the overall distribution of star-forming H 2 gas and its properties (Scoville & Solomon 1975;Sanders et al 1985;Dame & Thaddeus 1985;Scoville et al 1987;Clemens et al 1988;Matsunaga et al 2001;Dame et al 2001;Jackson et al 2006). CO emission is ubiquitous at all Galactic longitudes in the inner Galaxy (|l| < 90 • ) and within 1 • latitude of the Galactic plane.…”
Section: Observed Properties Of Molecular Gasmentioning
confidence: 99%
“…11 of Kraemer et al 2010), and the infrared dark cloud IRDC G79.3+0.3 (hereafter the IRDC) towards the southern and western borders (Redman et al 2003). The local arm is seen tangentially in this direction (Dame & Thaddeus 1985;Rygl et al 2012), which makes it difficult to determine distances and to identify mutual associations among targets associated with the Cyg X region. An update of the information currently available and a brief discussion of the distance is presented below, in Sect.…”
Section: Introductionmentioning
confidence: 99%