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J/A+A/177/131  CaII and MgII excess flux density in cool stars  (Rutten, 1987)

Magnetic structure in cool stars. XII. Chromospheric activity and rotation of giants and dwarfs. Rutten R.G.M. <Astron. Astrophys. 177, 131 (1987)> =1987A&A...177..131R
ADC_Keywords: Stars, late-type ; Stars, dwarfs ; Stars, giant ; Magnitudes, absolute Keywords: stars: chromospheres of - stars: evolution of - stars: late-type - stars: rotation of Abstract: The relation between the CaII H and K line-tore flux density and rotation period is studied for a sample of 313 cool stars of luminosity classes ranging from II-III to V, and compared to similar relations for MgII h and k and soft X-ray. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 110 313 Sample of stars used in the determination of the rotation-activity relation refs.dat 154 36 References table3.dat 79 13 Overactive stars
See also: J/A+AS/124/359 : Ca II triplet lines in cool stars (Mallik 1997) J/A+A/325/1115 : Near-simultaneous ROSAT and Mt Wilson data (Piters+ 1997) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 13 A13 --- Name Star name (1) 15- 18 F4.2 mag B-V B-V colour index 20- 30 A11 --- SpType MK spectral type 33- 38 F6.2 d Per Rotation period 40 A1 --- r_Per [a-v] Reference for period, in refs.dat file (2) 43- 47 F5.2 mag VMAGp ? Absolute magnitude derived from parallax 50- 54 F5.2 mag VMAGw ? Absolute magnitude derived from Wilson-Bappu width 57- 61 F5.2 mag VMAGs ? Absolute magnitude derived from Stromgren photometry 65- 69 F5.2 mag VMAGg ? Absolute magnitude derived from Geneve photometry 72- 76 F5.2 mag VMAG Adopted mean absolute v magnitude 77 A1 --- n_VMAG [)] ): Absolute magnitudes determined from luminosity class 79- 82 F4.1 solRad Rad ? Stellar radius 85- 89 F5.2 mW/m2 DCaII CaII H and K line-core excess flux density 90 A1 --- n_DCaII [)] ): a correction has been applied for the M-type dwarfs 92 I1 10uW/m2 e_DCaII rms uncertainty on DCaII 94- 99 A6 --- r_DCaII Reference for DCaII, separated by comma, 101-105 F5.2 mW/m2 DMgII ? Mg II H&K excess flux density 107 I1 10uW/m2 e_DMgII ? rms uncertainty on DMgII 109-110 I2 --- r_DMgII ? Reference for DMgII, in refs.dat file
Note (1): Names: * BD (Cat. I/119, I/122) * gl (Gliese catalogue number, see Cat. V/70) * Hz (Hertzsprung number for Pleiades <Cl Melotte 22> in Simbad) * Vb (Van Bueren number for Hyades <Cl Melotte 25> in Simbad) Note (2): Period derived from: * a--e for CaII modulation periods, * f--i for orbital periods, * j--q for broad-band modulation periods and * v for periods estimated from vsini.
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 2 A2 --- Ref Reference code 4- 22 A19 --- BibCode BibCode 24- 43 A20 --- Aut Author's name 46-154 A109 --- Com Comments
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Star name (HD number) 12- 23 A12 --- OName Other name of the star 25- 28 F4.2 mag B-V B-V colour index 33- 47 A15 --- SpType MK spectral type 50- 54 F5.2 d Per Period 57- 60 F4.2 [mW/m2] logECaII log of CaII excess flux density 63- 66 F4.2 [mW/m2] log(EX) ? log of soft X-ray excess flux density 69- 79 A11 --- Rem Remarks
History: * 27-Jun-2003: Prepared via OCR at CDS. * 01-Feb-2014: Fixed error on record#299 of table2 (thanks to Saulius Raudeliunas) References: Middelkoop & Zwaan, Paper I 1981A&A...101...26M Tinbergen & Zwaan, Paper II 1981A&A...101..223T Middelkoop, Paper III 1981A&A...101..295M Middelkoop, Paper IV 1982A&A...107...31M Oranje et al., Paper V 1982A&A...110...30O Middelkoop, Paper VI 1982A&A...113....1M Rutten, Paper VII 1984A&A...130..353R Oranje & Zwaan, Paper VIII 1985A&A...147..265O Oranje, Paper IX 1986A&A...154..185O Rutten, Paper X 1986A&A...159..291R Schrijver, Paper XI 1987A&A...172..111S Rutten & Schrijver Paper XIII 1987A&A...177..155R Schrijver & Rutten Paper XIV 1987A&A...177..143S Rutten & Pylyser, Paper XV 1988A&A...191..227R Rutten et al., Paper XVI 1989A&A...219..239R Rutten et al., Paper XVII 1991A&A...252..203R Lemmens et al., Paper XVIII 1992A&A...257..671L
(End) James Marcout, Patricia Bauer [CDS] 27-Jun-2003
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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