Access to Astronomical Catalogues

← Click to display the menu
J/MNRAS/369/783  Radial velocities & distances of carbon stars (Menzies+, 2006)

Carbon-rich Mira variables: radial velocities and distances. Menzies J.W., Feast M.W., Whitelock P.A. <Mon. Not. R. Astron. Soc., 369, 783-790 (2006)> =2006MNRAS.369..783M
ADC_Keywords: Stars, carbon ; Radial velocities ; Stars, distances Keywords: stars: AGB and post-AGB - stars: carbon - stars: distances - stars: variables: other - Galaxy: kinematics and dynamics Abstract: Optical radial velocities have been measured for 38 C-type Mira variables (C-Miras). These data together with others in the literature are used to study the differences between optical and CO millimetre (mm) observations for C-Miras and the necessary corrections to the optical velocities are derived in order to obtain the true radial velocities of the variables. The difference between absorption and emission-line velocities is also examined. A particularly large difference (+30km/s) is found in the case of the Hα line. A catalogue is given of 177 C-Miras with estimated distances and radial velocities. The distances are based on bolometric magnitudes derived in Paper I (Whitelock et al., 2006, Cat. J/MNRAS/369/751) using South African Astronomical Observatory (SAAO) observations or (for 60 of the stars) using non-SAAO photometry. In the latter case, the necessary transformations to the SAAO system are derived. These data will be used in Paper III (Feast et al., 2006MNRAS.369..791F) to study the kinematics of the C-Miras. Description: All SAAO spectra were obtained with the Unit Spectrograph attached to the 1.9-m telescope at Sutherland. A SITe 1798x266-pixel CCD with 13-m pixels was used in the spectrograph camera. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 41 68 New heliocentric radial velocities table3.dat 77 60 Non-SAAO photometry converted to the SAAO system table4.dat 52 177 Distance and velocity data
See also: J/MNRAS/369/751 : Near-infrared photometry of carbon stars (Whitelock+, 2006) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 13 A13 --- Name Star name 17- 21 F5.1 km/s Vabs ? Absorption velocity 26- 31 F6.2 km/s Vem ? Emission velocity 33- 41 F9.1 d JD Julian date of observation
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Star name 18- 27 A10 --- IRAS IRAS number 29- 33 F5.2 mag Jmag ? J magnitude 35- 39 F5.2 mag Hmag ? H magnitude 41- 45 F5.2 mag Kmag ? K magnitude 47- 51 F5.2 mag Lmag ? L magnitude (3.5µm) 53- 56 F4.2 mag AV Absorption in V band 58- 61 F4.2 mag mbol Bolometric apparent magnitude 63- 64 I2 --- NIR Number of near-IR observations used 66- 68 I3 d Per Period 70 A1 --- r_Per Source for Period if not GCVS (1) 72- 75 A4 --- r_NIR Source for near-IR observations (1) 77 A1 --- MSX [X] X when MSX data were used
Note (1): Source for periods if not GCVS and near-IR observations as follows: A = Pojmaski (2003AcA....53..341P) & Pojmaski & Maciejewski (2004AcA....54..153P), Cat. II/264. B = Le Bertre (1992A&AS...94..377L) C = mean of J and N; G = Groenewegen et al. (1998MNRAS.293...18G) J = Jones et al. (1990ApJS...74..785J) H = Perryman et al., HIP (1997, Cat. I/239) N = Nakashima et al. (2000PASJ...52..275N) O = Olivier, Whitelock & Marang (2001MNRAS.326..490O) D = Dahlmark (1993IBVS.3855....1D, 1996IBVS.4329....1D) Cat. II/238 M = 2MASS, Cat. II/246 P = Noguchi et al. (1981PASJ...33..373N) T = Taranova & Shenavrin (2004, Cat. J/PAZh/30/605>) E = ESO (see Section 4) S = SAAO from Paper I, Whitelock et al., 2006, Cat. J/MNRAS/369/751
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1 I1 --- n_Name [1/3] JHKL photometry (1) 3- 18 A16 --- Name Star name 19- 23 F5.2 kpc Dist1 Distance for ZP=1.87 (2) 25- 28 F4.2 mag AV1 Absorption in V band for ZP=1.87 (2) 30- 34 F5.2 kpc Dist2 Distance for ZP=2.06 (3) 36- 39 F4.2 mag AV2 Absorption in V band for ZP=2.06 (3) 41- 43 I3 d Per Period 45- 50 F6.1 km/s Vlsr LSR velocity 52 A1 --- n_Vlsr [co] Vlsr determined from from (c) CO mm or (o) optical/near-IR
Note (1): Note as follows: 1 = Stars with JHKL photometry in Paper I, (Whitelock et al., 2006, Cat. J/MNRAS/369/751 3 = Stars with JHKL photometry in Table 3 Note (2): Zero-point is derived from an adopted LMC modulus of 18.50 Note (3): Zero-point derived in Paper III (Feast et al., 2006MNRAS.369..791F) is used
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 19-Jan-2007
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

catalogue service

© UDS/CNRS

Contact