J/A+A/542/A33       3 M dwarfs near-infrared spectra         (Onehag+, 2012)

M dwarf metallicities. A high-resolution spectroscopic study in the near-infrared. Onehag A., Heiter U., Gustafsson B., Piskunov N., Plez B., Reiners A. <Astron. Astrophys. 542, A33 (2012)> =2012A&A...542A..33O 2012A&A...542A..33O
ADC_Keywords: Stars, dwarfs ; Stars, M-type ; Spectra, infrared Keywords: stars: atmospheres - stars: binaries visual - stars: low-mass - stars: abundances - techniques: spectroscopic Abstract: The relatively large spread in the derived metallicities ([Fe/H]) of M dwarfs shows that various approaches have not yet converged to consistency. The presence of strong molecular features, and incomplete line lists for the corresponding molecules have made metallicity determinations of M dwarfs difficult. Furthermore, the faint M dwarfs require long exposure times for a signal-to-noise ratio sufficient for a detailed spectroscopic abundance analysis. We present a high-resolution (R∼50000) spectroscopic study of a sample of eight single M dwarfs and three wide-binary systems observed in the infrared J-band. Description: The observations were carried out in service mode with the infrared spectrometer CRIRES at ESO-VLT. In total 14 targets were observed during periods 82 (1st of October 2008 to 31st of March 2009) and 84 (1st of October 2009 to 31st of March 2010). Objects: ---------------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------------- 11 42 10.55 +26 42 30.5 GJ 436 = HIP 57087 (fig1.dat) 06 52 18.05 -05 10 25.4 GJ 250A = HIP 32984 (fig2.dat) 06 52 18.05 -05 11 24.2 GJ 250B = TYC 4808-765-1 (fig3.dat) 22 09 40.34 -04 38 26.6 GJ 849 = HIP 109388 (fig4.dat) ---------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file fig1.dat 71 655 Synthetic and observed spectra for GJ 436 fig2.dat 45 8168 Synthetic and observed spectra for GJ 250A fig3.dat 45 8168 Synthetic and observed spectra for GJ 250B fig4.dat 45 8168 Synthetic and observed spectra for GJ 849 -------------------------------------------------------------------------------- Byte-by-byte Description of file: fig1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Panel [1/2] Panel number 8- 16 F9.3 0.1nm lambda [11953/11998] Wavelength 23- 32 F10.8 --- Flux Normalized flux 38- 45 F8.6 --- Fit Synthetic fit, with adopted Teff=3263K 51- 58 F8.6 --- Fit-200 Synthetic fit, with adopted Teff=3263-200K 64- 71 F8.6 --- Fit+200 Synthetic fit, with adopted Teff=3263+200K -------------------------------------------------------------------------------- Byte-by-byte Description of file: fig2.dat fig3.dat fig4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Seg [1/8] Seg number 8- 16 F9.3 0.1nm lambda [11373/13059] Wavelength 23- 32 F10.8 --- Flux Normalized flux 38- 45 F8.6 --- Fit Synthetic fit -------------------------------------------------------------------------------- Acknowledgements: Anna Onehag, Anna.Onehag(at)fysast.uu.se
(End) Patricia Vannier [CDS] 18-Jun-2012
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