J/A+A/275/163      Luminous Carbon stars in Galactic Plane  (Kastner+ 1993)

Probing the AGB tip: luminous carbon stars in the galactic plane Kastner J.H., Forveille T., Zuckerman B., Omont A. <Astron. Astrophys. 275, 163 (1993)> =1993A&A...275..163K 1993A&A...275..163K
ADC_Keywords: Stars, peculiar; CO; Radio lines Keywords: surveys - stars: carbon - stars: AGB - stars: evolution - circumstellar matter - radio lines: stars Description: A sample of distant (2-10kpc), heavily obscured asymptotic giant branch (AGB) stars were observed for CO emission. Simultaneous observations at the frequencies of the J=1-0 (115.27GHz) and J=2-1 (230.58GHz) transitions of CO were made at the 30m IRAM telescope on Pico Velata, Spain, in September 1989. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 101 61 Sources observed in CO table2.dat 56 61 CO observations: results table3.dat 74 45 Near-IR photometry of CO sources table4.dat 38 20 Detections of SiO, H2O and HCN table5.dat 71 49 Kinematic distances, bolometric fluxes, luminosities -------------------------------------------------------------------------------- Byte-per-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- IRAS IRAS name 14- 15 I2 h RAh Right ascension (1950) 17- 18 I2 min RAm Right ascension (1950) 20- 23 F4.1 s RAs Right ascension (1950) 27 A1 --- DE- Declination sign 28- 29 I2 deg DEd Declination (1950) 31- 32 I2 arcmin DEm Declination (1950) 34- 35 I2 arcsec DEs Declination (1950) 39- 41 I3 deg GLON Galactic longitude (lII) 45- 48 F4.1 deg GLAT Galactic latitude (bII) 51- 62 A12 Jy Flux IRAS fluxes: F12,F25,F60 64- 65 A2 --- LRS IRAS LRS type (1) 69- 70 I2 % Var IRAS variability index 72-105 A34 --- Name Other object designations -------------------------------------------------------------------------------- Note (1): Letter designations refer to classification in Volk et al., 1991ApJS...77..607V 1991ApJS...77..607V: I = noisy/incomplete, F = featureless C = SiC emission, E = silicate emission U = unusual See also the IRAS LRS (Cat. III/197) -------------------------------------------------------------------------------- Byte-per-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- IRAS IRAS name 14- 17 F4.2 K.km/s TB.V(1-0) ? CO(1-0) 115.27GHz line area 19 A1 --- l_TB.V(1-0) ? CO(1-0) upper limit flag 20- 23 F4 K TB(1-0) ? CO(1-0) peak antenna temperature TB 26- 28 I3 km/s V(LSR)(1-0) ? CO(1-0) LSR velocity 32- 33 I2 km/s Vexp(1-0) ? CO(1-0) expansion velocity 37- 41 F5.2 K.km/s TB.V(2-1) ? CO(2-1) 230.54GHz line area 42 A1 --- l_TB.V(2-1) ? CO(2-1) upper limit flag 43- 46 F4 K TB(2-1) ? CO(2-1) peak antenna temperature TB 49- 51 I3 km/s V(LSR)(2-1) ? CO(2-1) LSR velocity 55- 56 I2 km/s Vexp(2-1) ? CO(2-1) expansion velocity -------------------------------------------------------------------------------- Byte-per-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- IRAS IRAS name 12- 18 F7.1 mJy J ? J(1.25 micron) flux, uncorrected 20- 26 F7.1 mJy H ? H(1.65 micron) flux, uncorrected 28- 34 F7.1 mJy K ? K(2.2 micron) flux, uncorrected 36- 40 I5 mJy L ? L(3.5 micron) flux, uncorrected 43- 49 F7.1 mJy Jc ? J(1.25 micron) flux, corrected 51- 57 F7.1 mJy Hc ? H(1.65 micron) flux, corrected 59- 66 F8.1 mJy Kc ? K(2.2 micron) flux, corrected 67- 72 I6 mJy Lc ? L(3.5 micron) flux, corrected 74 I1 --- r_flux ? Reference flag (1) -------------------------------------------------------------------------------- Note (1): Photometry obtained at Kitt Peak 2.1-meter telescope except where noted: 1 : S. G. Kleinmann, private communication 2 : Epchtein et al., 1990A&A...227...82E 1990A&A...227...82E 3 : Epchtein et al., in preparation (data for 03301+5658 are of poor quality) 4 : Guglielmo et al., 1993, A&AS (in press) 1993A&AS...99...31G 1993A&AS...99...31G -------------------------------------------------------------------------------- Byte-per-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- IRAS IRAS name 14- 16 A3 --- Molecule Molecule name 20- 24 F5.3 K TB Peak antenna temperature TB 26- 30 F5.1 km/s Vlsr LSR velocity 34- 38 F5.2 km/s DeltaV Line width (1) -------------------------------------------------------------------------------- Note (1): the line width is: for SiO and H2O detection: full width at half maximum, for HCN: half width at zero power -------------------------------------------------------------------------------- Byte-per-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- IRAS IRAS name 14- 15 A2 --- Type AGC type (C or O) 17- 20 F4.1 kpc Dkin ? Near kinematic distance 24- 29 E6.1 mW/m2 Fbol ? Bolometric flux, uncorrected 33- 37 E5.1 solLum L ? Luminosity, uncorrected 41- 46 E6.1 mW/m2 Fbol,0 ? Bolometric flux, corrected 50- 54 E5.1 solLum L0 ? Luminosity, corrected 58- 63 E6.1 mW/m2 Fbol,BC ? Bolometric flux from (12-25) color 67- 71 E5.1 solLum LBC ? Luminosity from (12-25) color -------------------------------------------------------------------------------- History: * 14-Jul-2001 [CDS]: table1 corrected from a folded lines version.
(End) Patricia Bauer [CDS] 21-Sep-1993
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