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J/A+A/317/761       Miras temperatures, distances & magnitudes (Alvarez+ 1997)

Determination of Miras temperatures from TiO and VO bands. Estimates of distances. Alvarez R., Mennessier M.-O. <Astron. Astrophys. 317, 761 (1997)> =1997A&A...317..761A (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable ; Models, atmosphere Keywords: stars: atmospheres - stars: distances - stars: fundamental parameters - stars: AGB and post-AGB - Description: Effective temperatures are determined for a sample of 165 oxygen-rich Miras using indices related to molecular band strength of titanium oxide and vanadium oxide. Using a theoretical evolutionary track on AGB, absolute bolometric magnitudes are computed. Apparent bolometric magnitudes are determined from narrow-band photometry observations. They are used to calibrate distances. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2 61 165 Fundamental parameters
Byte-by-byte Description of file: table2
Bytes Format Units Label Explanations
1- 6 A6 --- GCVS Name 10- 12 I3 d P Period 16- 17 A2 --- Group Group 21- 24 I4 K T Temperature 28- 30 I3 K e_T Uncertainty on temperature 34- 36 I3 K Amp Amplitude of temperature variation 40- 43 F4.1 mag Mbol Absolute bolometric magnitudes 47- 49 F3.1 mag mbol Apparent bolometric magnitudes 52- 55 I4 pc Dist Distance 60- 61 A2 --- Type Mira type, see Note (1)
Note (1): the type is defined as: H: Miras classified as halo stars by Luri et al. (1996A&AS..117..405L) SP: Short-period Miras not belonging to the sample of Luri et al. MS: MS-Miras
Acknowledgements: R. Alvarez References: Luri X., Mennessier M-O., Torra J., Figueras F., 1996, Astron. Astrophys., Suppl. Ser., 117, 405
(End) Alvarez [GRAAL], Patricia Bauer [CDS] 10-Jun-1996
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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