J/ApJS/161/361    Millimeter continuum survey for protoclusters   (Klein+, 2005)

A millimeter continuum survey for massive protoclusters in the outer Galaxy. Klein R., Posselt B., Schreyer K., Forbrich J., Henning T. <Astrophys. J. Suppl. Ser., 161, 361-393 (2005)> =2005ApJS..161..361K 2005ApJS..161..361K
ADC_Keywords: Millimetric/submm sources ; Infrared sources Keywords: stars: formation - submillimeter - surveys Abstract: Our search for the earliest stages of massive star formation turned up 12 massive pre-protocluster candidates plus a few protoclusters. For this search, we selected 47 FIR-bright IRAS sources in the outer Galaxy. We mapped regions of several square arcminutes around the IRAS source in the millimeter continuum in order to find massive cold cloud cores possibly being in a very early stage of massive star formation. Masses and densities are derived for the 128 molecular cloud cores found in the obtained maps. Description: The millimeter continuum maps were collected at three observatories: the Heinrich Hertz Submillimeter Telescope (SMT, Mount Graham, Arizona), the Institut de Radioastronomie Millimetrique (IRAM) 30m telescope (Pico Veleta, Spain), and the James Clerk Maxwell Telescope (JCMT, Mauna Kea, Hawaii). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 70 47 Source list table4.dat 52 7 The observing runs table56.dat 92 137 Source components -------------------------------------------------------------------------------- See also: J/A+AS/115/81 : A CS(2-1) survey of UC HII regions (Bronfman+, 1996) J/A+AS/143/269 : 6.7GHz methanol maser emission survey (Szymczak+, 2000) J/A+A/368/845 : Arcetri Catalog of H2O maser sources. Update. (Valdettaro+, 2001) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- IRAS IRAS name 12- 15 F4.2 kpc Dist Distance 16 A1 --- f_Dist [a] Indicates a photometric distance 17- 25 A9 [solLum] Lum Luminosity (1) 27- 30 F4.1 K Tdust Dust temperature (1) 32- 68 A37 --- ONames Other designations 70 I1 --- Ref Reference (2) -------------------------------------------------------------------------------- Note (1): From Schreyer et al. (1996A&A...306..267S 1996A&A...306..267S) Note (2): Reference number, defined as follows: 1 = Henning et al. (1992A&AS...93..525H 1992A&AS...93..525H) 2 = Bronfman et al. (1996, Cat. J/A+AS/115/81) 3 = Schreyer (1997, Ph.D. thesis, Univ. Jena) 4 = Mueller et al. (2002ApJS..143..469M 2002ApJS..143..469M) 5 = Szymczak et al. (2000, Cat. J/A+AS/143/269) 6 = Valdettaro et al. (2001, Cat. J/A+A/368/845) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Run Observing run number 3- 6 A4 --- Tel Telescope 8- 21 A14 --- Inst Instrument 23- 25 I3 GHz Freq Frequency 27- 28 I2 GHz DFreq Frequency width 30- 41 A12 --- ObsDate Date of observation 43- 46 F4.1 arcsec FWHM Full width at half maximum 48- 52 F5.1 mJy rms Noise rms (in units of mJy/beam) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table56.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- IRAS IRAS name 11- 12 A2 --- m_IRAS [/1-9] Merged IRAS name 14 I1 --- Run Observing run number 16- 18 I3 GHz Freq Frequency 20- 21 A2 --- Comp Source component 23- 27 F5.2 Jy Fint ? Mean integrated flux density at Freq 29- 33 F5.2 Jy e_Fint ? Error in Fint 35- 39 I5 arcsec2 Aint ? Mean integration area 41- 45 F5.2 Jy Fpeak ? Peak flux density at Freq (in units of Jy/θbeam) 47- 49 I3 mJy sigma σ level of the map (in units of mJy/θbeam) 51- 54 F4.2 pc theta ? Component extension θsource derived from Aint (beam-deconvolved angular diameter of the source) 55 A1 --- f_theta [a] Flag on theta (1) 57- 60 I4 solMass Mgas ? Gas mass 62- 65 F4.1 10+22cm-2 NH ? Column density N(H) 67- 71 F5.1 10+4cm-3 nH ? Number density n(H) 73- 74 I2 h RAh ? Hour of Right Ascension (B1950) (2) 76- 77 I2 min RAm ? Minute of Right Ascension (B1950) (2) 79- 82 F4.1 s RAs ? Second of Right Ascension (B1950) (2) 84 A1 --- DE- Sign of the Declination (B1950) (2) 85- 86 I2 deg DEd ? Degree of Declination (B1950) (2) 88- 89 I2 arcmin DEm ? Arcminute of Declination (B1950) (2) 91- 92 I2 arcsec DEs ? Arcsecond of Declination (B1950) (2) -------------------------------------------------------------------------------- Note (1): A "a" indicates that the beam area is larger than the source extent, and it is used for further calculations. Note (2): Peak position -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Marianne Brouty [CDS] 20-Sep-2006
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