2001
DOI: 10.1086/320404
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[ITAL]MIDCOURSE SPACE EXPERIMENT[/ITAL][ITAL]Midcourse Space Experiment[/ITAL] Survey of the Galactic Plane

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Cited by 480 publications
(419 citation statements)
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“…When the distance ambiguity could be solved, the preferred distance and mass are shown in boldface. searched systematically for infrared counterparts to our preliminary catalog of 6000 sources in the IRAS Point Source Catalog (Beichman et al 1988) and in the Midcourse Space Experiment (MSX, Price et al 2001) data, using a search radius of 30 (more details will be given in Contreras et al, in prep.). Only ∼10% of the submm compact sources can be associated with an IRAS point source, and ∼32% have a possible MSX counterpart (Fig.…”
Section: Nature Of the Sourcesmentioning
confidence: 99%
“…When the distance ambiguity could be solved, the preferred distance and mass are shown in boldface. searched systematically for infrared counterparts to our preliminary catalog of 6000 sources in the IRAS Point Source Catalog (Beichman et al 1988) and in the Midcourse Space Experiment (MSX, Price et al 2001) data, using a search radius of 30 (more details will be given in Contreras et al, in prep.). Only ∼10% of the submm compact sources can be associated with an IRAS point source, and ∼32% have a possible MSX counterpart (Fig.…”
Section: Nature Of the Sourcesmentioning
confidence: 99%
“…(This table is available in its entirety in FITS format.) 10 Bright, massive YSO candidates in M17 SWex detected by The Midcourse Space Experiment (MSX; Price et al 2001) were previously cataloged by PW10; we incorporate three of these sources into our analysis of the M17 SWex stellar population in the ACIS FOV (Section 3). 11 This essentially leaves A V unconstrained when fitting sources with YSO models, necessary because candidate protostars are found deeply embedded in the IRDC lanes, where extinction can be extreme and background stars are obscured even in the IR.…”
Section: A1 Mir Identification Of Ysos Associated With M17 Swexmentioning
confidence: 99%
“…The panel at lower right shows (red) contours of the peak CO brightness over the wider range −26 km s −1 < v < 26 km s −1 overlaid on an image of MSX (Price et al 2001) Band A 8.3μ emission.…”
Section: Disk and Bar Gas Atmentioning
confidence: 99%