J/ApJ/682/L117          A spectroscopic orbit for Regulus          (Gies+, 2008)

A spectroscopic orbit for Regulus. Gies D.R., Dieterich S., Richardson N.D., Riedel A.R., Team B.L., McAlister H.A., Bagnuolo W.G.Jr, Grundstrom E.D., Stefl S., Rivinius T., Baade D. <Astrophys. J., 682, L117-L120 (2008)> =2008ApJ...682L.117G 2008ApJ...682L.117G
ADC_Keywords: Binaries, spectroscopic ; Stars, B-type ; Radial velocities Keywords: binaries: spectroscopic - stars: early-type - stars: individual (Regulus, α Leonis) Abstract: We present a radial velocity study of the rapidly rotating B star Regulus that indicates the star is a single-lined spectroscopic binary. The orbital period (40.11 days) and probable semimajor axis (0.35AU) are large enough that the system is not interacting at present. However, the mass function suggests that the secondary has a low mass (M2>0.30M), and we argue that the companion may be a white dwarf. Such a star would be the remnant of a former mass donor that was the source of the large spin angular momentum of Regulus itself. Description: Table 1 lists the sources and properties of the spectra of Regulus used to measure radial velocity. The spectra from run numbers 1-8 were made by us and have moderate resolving power and good S/N (usually better than 100 per pixel). Other spectra are from online archives. Objects: --------------------------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------------------------- 10 08 22.3 +11 58 02 NAME REGULUS = * alf Leo = HIP 49669 --------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 71 15 Journal of spectroscopy table2.dat 35 168 Radial velocity measurements -------------------------------------------------------------------------------- See also: III/252 : Pulkovo radial velocities for 35493 HIP stars (Gontcharov, 2006) III/190 : WEB Catalog of Radial Velocities (Duflot+ 1995) J/MNRAS/389/869 : Multiplicity among bright stellar systems (Eggleton+, 2008) J/AJ/133/889 : Faint companions of Hipparcos stars (Lepine+, 2007) J/ApJ/663/960 : Radial velocities of Leo I stars (Sohn+, 2007) J/AJ/126/2048 : NStars project: the Northern Sample. I. (Gray+, 2003) J/A+A/379/162 : Binaries with post-T Tauri secondaries (Gerbaldi+, 2001) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Seq Running sequence number 4- 9 F6.1 yr Date1 Date of observation in Besselian year (first) 10 A1 --- --- [-] 11- 16 F6.1 yr Date2 ? Date of last observation in Besselian year 18- 36 A19 0.1nm Range Range in Angstrom 38- 43 I6 --- Power Resolving power (λ/Δλ) 45- 46 I2 --- Nsp Number of observed spectra 48- 71 A24 --- Tel Observatory/Telescope/Spectrograph -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.3 d Date HJD 13- 17 F5.3 -- Phase Orbital phase from ascending node 19- 22 F4.1 km/s HRV Heliocentric radial velocity 24- 27 F4.1 km/s e_HRV Mean error on HRV 29- 32 F4.1 km/s O-C Observed minus calculated residual 34- 35 I2 -- Seq Running sequence number from Table 1 -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 04-Nov-2010
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