J/A+A/550/A70 Galactic and Magellanic Cloud Cepheids distance (Groenewegen 2013)

Baade-Wesselink distances to Galactic and Magellanic Cloud Cepheids and the effect of metallicity. Groenewegen M.A.T. <Astron. Astrophys., 550, A70 (2013)> =2013A&A...550A..70G 2013A&A...550A..70G
ADC_Keywords: Milky Way ; Magellanic Clouds ; Stars, variable ; Stars, distances Keywords: stars: distances - stars: variables: Cepheids Abstract: The metallicity dependence of the Cepheid period-luminosity (PL) relation is of importance in establishing the extragalactic distance scale. The aim of this paper is to investigate the metallicity dependence of the PL relation in V and K, based on a sample of 128 Galactic, 36 Large Magellanic Cloud (LMC), and 6 Small Magellanic Cloud (SMC) Cepheids with individual Baade-Wesselink (BW) distances (some of the stars also have an Hubble Space Telescope (HST) based and Hipparcos parallax or are in clusters) and individually determined metallicities from high-resolution spectroscopy. Literature values of the V-band, K-band, and radial velocity data were collected for the sample of Cepheids. Based on a (V-K) surface-brightness relation and a projection factor, distances were derived from a BW analysis. Since 2008, additional radial velocity data has been obtained using the 1.2m Euler telescope located at the La Silla observatory (see Groenewegen 2008A&A...488...25G 2008A&A...488...25G for a description of the data taking and data reduction). The new Radial Velocity (RV) data are presented in Table 3. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table10.dat 109 170 *Distances, radii, and absolute magnitudes from the Baade-Wesselink (BW) analysis table3.dat 29 170 *New radial velocity data table45.dat 25 143 Published [Fe/H] values for Cepheids tablea1.dat 40 23 Distances to cluster containing Cepheids notes.dat 80 61 Notes to tablea1 -------------------------------------------------------------------------------- Note on table10.dat, table5.dat: X Sct was observed for radial velocities (table3.dat), but has too poor near-IR data for BW analysis, and is therefore absent from table10.dat -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Loc [GLS] Localisation: Galaxy / LMC / SMC 3- 11 A9 --- Name Cepheid name 13- 17 F5.3 mag E(B-V) Colour excess 19- 23 F5.3 mag e_E(B-V) rms uncertainty on E(B-V) 25- 33 F9.6 d Per Period 35- 39 F5.3 --- p p-factor relation (p=1.50-0.24logPer) 41- 47 F7.1 pc Dist Cepheid distance 49- 54 F6.1 pc e_Dist Error in the fit on Dist 56- 61 F6.1 pc e.D Error based on Monte-Carlo simulation on Dist 63- 67 F5.1 Rsun Rad Cepehid radius 69- 72 F4.1 Rsun e_Rad Error in the fit on Rad 74- 77 F4.1 Rsun e.R Error based on Monte-Carlo simulation on Rad 79- 83 F5.2 mag VMAG Absolute V magnitude 85- 88 F4.2 mag e_VMAG Error due to the errors of Dist and E(B-V) on VMAG 90- 93 F4.2 mag e.V Error based on Monte-Carlo simulation on VMAG 95- 99 F5.2 mag KMAG Absolute K magnitude 101-104 F4.2 mag e_KMAG Error due to the errors of Dist and E(B-V) on KMAG 106-109 F4.2 mag e.K Error based on Monte-Carlo simulation on KMAG -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Cepheid name 11- 22 F12.4 d JD Julian date 24- 29 F6.2 km/s RV Radial velocity -------------------------------------------------------------------------------- Byte-by-byte Description of file: table45.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Loc [GLS] Localisation: Galaxy / LMC / SMC 3- 11 A9 --- Name Cepheid name 14- 18 F5.2 [Sun] [Fe/H] Metallicity 20- 23 F4.2 [Sun] e_[Fe/H] ? rms uncertainty on [Fe/H] 25 I1 --- r_[Fe/H] Reference for [Fe/H] (1) -------------------------------------------------------------------------------- Note (1): References as follows: 1 = Luck & Lambert (2011, Cat. J/AJ/142/136) 2 = Luck et al. (2011, Cat. J/AJ/142/51) 3 = Romaniello et al. (2008A&A...488..731R 2008A&A...488..731R) 4 = Fry & Carney (1997, Cat. J/AJ/113/1073) 5 = Andrievsky et al. (2003AN....324..532A 2003AN....324..532A) 6 = Molinaro et al. (2012ApJ...748...69M 2012ApJ...748...69M) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Cepheid name 11- 23 A13 --- Cluster Cluster name 26- 30 F5.2 mag DM Adopted distance modulus for the cluster 32- 35 F4.2 mag e_DM rms uncertainty on DM 36 A1 --- n_DM [*] *: No error quoted, conservative error adopted 38- 40 A3 --- Met [BV JHK] Method of ZAMS fitting: with (B,V) or (J,H,K) colors. -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Cepheid name 11- 80 A70 --- Note Text of the note -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 30-Apr-2013
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