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J/A+A/379/305       Envelope Tomography of LPV stars        (Alvarez, 2001)

Envelope tomography of long-period variable stars. III. Line doubling frequency among Mira stars. Alvarez R., Jorissen A., Plez B., Gillet D., Fokin A., Dedecker M. <Astron. Astrophys. 379, 305 (2001)> =2001A&A...379..305A
ADC_Keywords: Stars, late-type ; Radial velocities Keywords: stars: AGB and post-AGB - stars: atmospheres - stars: late-type - stars: oscillations - stars: variables: general - shock waves Description: The table provides the heliocentric radial velocities (between parenthesis) for 81 Mira and semi-regular variables monitored at the Observatoire de Haute Provence with the ELODIE spectrograph. The different types of cross-correlation functions (CCFs) obtained with the K0 III- and M4 V-templates are coded as defined in the paper (see also Note 1 below). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 71 315 Heliocentric radial velocities and CCFs for 81 Mira and semi-regular variables
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Star name 10- 12 I3 solRad rho ? Stellar size; see Note (1) 14- 16 A3 --- Night Night number (see Table 2 of paper) 18- 26 F9.1 --- JD Julian date (middle of the night) 28- 31 F4.2 --- Phase ? Phase in the visual light cycle 32 A1 --- u_Phase [:] : to indicate uncertain phase 34- 36 A3 --- CCF(K0) Type of CCF with K0III template; see Note (2) 38- 43 F6.1 km/s HRV1(K0) ? K0 III-template heliocentric radial velocity (blue peak if two peaks present) 46- 51 F6.1 km/s HRV2(K0) ? K0 III-template heliocentric radial velocity (red peak if two peaks present) 54- 56 A3 --- CCF(M4) Type of CCF with M4V template; see Note (2) 58- 63 F6.1 km/s HRV1(M4) ? M4 V-template heliocentric radial velocity (blue peak if two peaks present) 66- 71 F6.1 km/s HRV2(M4) ? M4 V-template heliocentric radial velocity (red peak if two peaks present)
Note (1): rho is an estimate of the stellar size, through the relation rho = sqrt(L/Teff4) (in solar units). Not provided for S or C stars. Note (2): Type of cross-correlation function: 1p: single peak 2p: double peak ap: asymmetrical peak 1p?: doubtful single peak 2p?: doubtful double peak np: noisy profile
Acknowledgements: Alain Jorissen References: Alvarez et al., Paper I 2000A&A...362..655A Knapp et al., Paper II 2001A&A...371..222K
(End) Patricia Bauer [CDS] 11-Oct-2001
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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