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J/ApJ/606/L73       CO emission of 5 Herbig Ae stars         (Blake+, 2004)

High-resolution 4.7 micron Keck/NIRSPEC spectroscopy of the CO emission from the disks surrounding Herbig Ae stars. Blake G.A., Boogert A.C.A. <Astrophys. J., 606, L73-L76 (2004)> =2004ApJ...606L..73B
ADC_Keywords: Stars, A-type ; Stars, emission ; Infrared sources ; Carbon monoxide Keywords: infrared: ISM - ISM: molecules - planetary systems: protoplanetary disks - stars: formation Abstract: We explore the high-resolution (Λ/ΔΛ=25000;Δv=12km/s) M-band (4.7-5.1µm) spectra of several disk-dominated Herbig Ae (HAe) systems: AB Aur, MWC 758, MWC 480, HD 163296, and VV Ser. Description: The Herbig Ae stars AB Aur (spectral type A0), MWC 480 (A5), MWC 758 (A8), HD 163296 (A1), and VV Ser (A0) were observed with NIRSPEC at the Keck II telescope on several observing runs between 2001 January and 2003 July. Objects: ---------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------- 04 55 45.8 +30 33 04 AB Aur = HD 31293 04 58 46.3 +29 50 37 MWC 480 = HD 31648 05 30 27.5 +25 19 57 MWC 758 = HD 36112 17 56 21.3 -21 57 22 HD 163296 = EM* MWC 275 18 28 49.0 +00 08 39 VV Ser = HBC 282 ---------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 57 223 Observed CO line parameters for Herbig Ae stars
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 6 A6 --- CO CO line 8- 16 A9 --- Star Star name 18- 32 A15 --- Trans Transition 34 A1 --- l_FWHM Upper 3σ limit flag on FWHM 35- 39 F5.1 km/s FWHM ? Full-Width at Half-Maximum 41- 46 F6.2 10-17W/m2 Flux ? Line flux 47- 49 F3.1 10-17W/m2 e_Flux ? The 1σ error in Flux 51- 57 A7 --- Notes Additional notes (1)
Note (1): Additional notes as follows: 1 = severely affected by telluric lines 2 = some telluric residuals 3 = incomplete vdop coverage 4 = severe blending with H I emission 5 = line shape not Gaussian 6 = severe blend with CO P(1) 7 = blend with 12CO line 8 = deep central absorption, blanked in fits to line profiles
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 07-May-2004
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

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