J/other/ChA+A/36.238  Dense parts of outflows toward massive cores  (Sun+, 2012)

A sensitive survey of dense parts of outflows toward massive cores. Sun Y., Xu Y., Yang J. <Chinese Astron., 36, 238-245 (2012)> =2012ChA&A..36..238S 2012ChA&A..36..238S
ADC_Keywords: Associations, stellar ; Abundances ; Spectroscopy Keywords: stars: formation - radio continuum lines: ISM - ISM: abundances Abstract: A set of samples of 13 massive star-forming cores were observed in SiO (2-1), CH3OH (2-1) and C34S (2-1) thermal lines. Nine of these cores were detected in all three lines. Among the nine SiO detections, three were new detections, and relatively faint. Most of the lines have wide wings, which might be interpreted as the evidence of ongoing energetic outflows in the cores. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table14.dat 95 13 Observed samples and the RMS levels of each line after channel smoothing (table1) and column density and abundance (table4) table3.dat 113 42 Gaussian parameters of the detected lines with 1σ errors -------------------------------------------------------------------------------- Byte-by-byte Description of file: table14.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- Name Source name 16- 17 I2 h RAh Right ascension (J2000) 19- 20 I2 min RAm Right ascension (J2000) 22- 26 F5.2 s RAs Right ascension (J2000) 28 A1 --- DE- Declination sign (J2000) 29- 30 I2 deg DEd Declination (J2000) 32- 33 I2 arcmin DEm Declination (J2000) 35- 38 F4.1 arcsec DEs Declination (J2000) 40- 44 F5.3 K rms1 CH3OH(2-1) rms level 46- 50 F5.3 K rms2 C34S (2-1) rms level 52- 56 F5.3 K rms3 SiO (2-1) rms level 58- 61 F4.2 10+14cm-2 NSiO ? SiO column density 63- 66 F4.2 10+14cm-2 NCH3OH ? CH3OH column density 68- 72 F5.2 10+14cm-2 NC34S ? C34S column density 74- 77 F4.2 10+23cm-2 NH2 ? H2 column density 79- 83 F5.2 10-10 XSiO ? SiO abundance 85- 89 F5.2 10-10 XCH3OH ? CH3OH abundance 91- 95 F5.2 10-10 XC34S ? C34S abundance -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- Name Source name 16 I1 --- Line [1/4]? Line identification number (1) 18- 23 F6.2 km/s Vlsr1 ? CH3OH LSR velocity 25- 28 F4.2 km/s e_Vlsr1 ? rms uncertainty on CH3OH LSR velocity 30- 34 F5.2 km/s W1 ? CH3OH line width 36- 39 F4.2 km/s e_W1 ? rms uncertainty on CH3OH line width 41- 44 F4.2 K T*A1 ? CH3OH Antena temperature 46- 49 F4.2 K e_T*A1 ? rms uncertainty on CH3OH antenna temperature 51- 56 F6.2 km/s Vlsr2 ? C34S LSR velocity 58- 61 F4.2 km/s e_Vlsr2 ? rms uncertainty on C34S LSR velocity 63- 66 F4.2 km/s W2 ? C34S line width 68- 71 F4.2 km/s e_W2 ? rms uncertainty on C34S line width 73- 76 F4.2 K T*A2 ? C34S antenna temperature 78- 81 F4.2 K e_T*A2 ? rms uncertainty on C34S antenna temperature 83- 88 F6.2 km/s Vlsr3 ? C34S LSR velocity 90- 93 F4.2 km/s e_Vlsr3 ? rms uncertainty on C34S LSR velocity 95- 98 F4.2 km/s W3 ? C34S line width 100-103 F4.2 km/s e_W3 ? rms uncertainty on C34S line width 105-108 F4.2 K T*A3 ? C34S Antena temperature 110-113 F4.2 K e_T*A3 ? rms uncertainty on C34S Antena temperature -------------------------------------------------------------------------------- Note (1): Observed lines: ------------------------------------------------- Line Species Transition Rest Frequency Tsyst (MHz) (K) ------------------------------------------------- 1 CH3OH 21-11 E 96739.3630 130 2 CH3OH 20-10 A 96741.3770 130 3 CH3OH 20-10 E 96744.5490 130 4 CH3OH 21-11 E 96755.5070 130 C34S 2-1 96412.9610 130 SiO 2-1 v=0 86847.0100 210 ------------------------------------------------- -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 24-Dec-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line