J/ApJ/922/163  Opt. interferometry of G-M stars & V-K colors  (van Belle+, 2021)

Direct measurements of giant star effective temperatures and linear radii: calibration against spectral types and V-K color. van Belle G.T., von Braun K., Ciardi D.R., Pilyavsky G., Buckingham R.S., Boden A.F., Clark C.A., Hartman Z., van Belle G., Bucknew W., Cole G. <Astrophys. J., 922, 163 (2021)> =2021ApJ...922..163V 2021ApJ...922..163V
ADC_Keywords: Stars, G-type; Stars, K-type; Stars, M-type; Interferometry; Spectral types; Effective temperatures; Colors; Stars, diameters; Stars, masses; Optical; Infrared sources Keywords: Fundamental parameters of stars ; Red giant stars ; Stellar properties ; Stellar radii ; Calibration ; Long baseline interferometers ; Optical interferometry ; Stellar masses ; Interferometry ; High angular resolution ; Stellar effective temperatures ; Flux calibration Abstract: We calculate directly determined values for effective temperature (Teff) and radius (R) for 191 giant stars based upon high-resolution angular size measurements from optical interferometry at the Palomar Testbed Interferometer. Narrow- to wideband photometry data for the giants are used to establish bolometric fluxes and luminosities through spectral energy distribution fitting, which allows for homogeneously establishing an assessment of spectral type and dereddened V0-K0 color; these two parameters are used as calibration indices for establishing trends in Teff and R. Spectral types range from G0III to M7.75III, V0-K0 from 1.9 to 8.5. For the V0-K0={1.9,6.5} range, median Teff uncertainties in the fit of effective temperature versus color are found to be less than 50K; over this range, Teff drops from 5050 to 3225K. Linear sizes are found to be largely constant at 11R from G0III to K0III, increasing linearly with subtype to 50R at K5III, and then further increasing linearly to 150R by M8III. Three examples of the utility of this data set are presented: first, a fully empirical Hertzsprung-Russell diagram is constructed and examined against stellar evolution models; second, values for stellar mass are inferred based on measures of R and literature values for logg; finally, an improved calibration of an angular size prediction tool, based upon V and K values for a star, is presented. Description: The Palomar Testbed Interferometer (PTI) was an 85-110m baseline H- and K-band (1.6 and 2.2um) interferometer located at Palomar Observatory in San Diego County, California. The data from PTI considered herein cover the range from the beginning of 1998 (when the standardized data collection and pipeline reduction went into place) until the beginning of 2008 (when operations at PTI concluded). See Section 3. A large number of archival sources were researched for narrow- to broadband photometry. In addition to the archival sources, we engaged in an extensive program of photometric observing at the Lowell 31 inch telescope located at Anderson Mesa. These visible data included broadband Johnson UBVRI, as well as narrowband photometry taken in the Hale-Bopp (HB) system of Farnham+ (2000Icar..147..180F 2000Icar..147..180F). See Section 4.2. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 127 256 Computed bolometric fluxes for the program stars table6.dat 64 9632 Photometry for the program stars table9.dat 69 191 Angular sizes, UD sizes, limb darkening corrections, unreddened V0-K0 color, and computed effective temperatures for the program stars table10.dat 76 191 Luminosities L and radii R for the program stars table20.dat 64 211 Broadband H- and K-band angular sizes for the program stars table21.dat 65 91 Reported logg values for the program stars found in the PASTEL catalog (2020-01-30 version) of Soubiran+ (2016A&A...591A.118S 2016A&A...591A.118S ; Cat. B/pastel) along with resulting mass determinations M. -------------------------------------------------------------------------------- See also: B/pastel : The PASTEL catalogue (Soubiran+, 2016-) B/mk : Catalogue of Stellar Spectral Classifications (Skiff, 2009- ) V/55 : A catalogue of high-velocity stars (Roman, 1955) II/5 : UBV Photometry of Bright Stars (Johnson+ 1966) II/21 : Narrow-Band Photometry of Late-Type Stars (Haeggkvist+ 1970) II/46 : Strong cyanogen stars (McClure 1970) III/106 : MK Classification of Visual Multiples (Abt, 1981) II/78 : uvby-Beta Phot 398 Members of Visual Multiple Systems (Olsen 1982) III/119 : Spectral classifications of proper motion stars (Bidelman+ 1985) III/150 : Perkins Revised MK Types for the Cooler Stars (Keenan+ 1989) II/164 : DDO Photoelectric Photometric Catalog (Mermilliod+ 1989) V/69 : MK, UBV Time and Latitude Stars (Sato+ 1990) V/81 : Taxonomy of Barium Stars (Lu 1991) II/182 : UBV Photometry of Stars with Accurate Positions (Oja 1984-1993) II/196 : Vilnius Photometry in two Nebulae (Straizys et al., 1993) II/215 : uvby-beta Catalogue (Hauck+ 1997) V/103 : NGP G5-M stars RV, DDO and BV photometry (Yoss+, 1997) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) J/ApJS/59/95 : Visual multiples. VIII. (Abt+, 1985) J/AJ/107/1556 : Late B-type stars classification (Garrison+, 1994) J/A+AS/106/397 : Sra and Srb semiregular variables (Kerschbaum+, 1994) J/ApJS/99/135 : Rotation and Spectral Peculiarities (Abt+ 1995) J/A+AS/113/441 : JHKL'M-photometry for 44 stars (Kerschbaum, 1995) J/A+AS/131/209 : JHK(L') photometry of giant stars (Alonso+ 1998) J/ApJS/119/83 : IUE sample of binaries with hot component (Parsons+, 1998) J/PASP/110/863 : Stellar Spectral Flux Library: 1150-25000Å (Pickles 1998) J/A+A/367/111 : A Hipparcos study of the Hyades cluster (de Bruijne+, 2001) J/ApJS/143/513 : Spectral classification of close binaries (Ginestet+, 2002) J/AJ/126/2048 : NStars project: the Northern Sample. I. (Gray+, 2003) J/ApJS/154/673 : COBE DIRBE Point Source Catalog (Smith+, 2004) J/A+A/475/1003 : Stellar parameters of G and K giant stars (Hekker+, 2007) J/A+A/469/713 : Chromospherically active stars in CoRoT (Medhi+, 2007) J/ApJS/176/216 : MK spectral types of Visual Multiples (Abt, 2008) J/AN/329/609 : Red giant candidates in 10 open clusters (Claria+, 2008) J/ApJS/176/276 : PTI calibrator catalog (van Belle+, 2008) J/ApJ/694/1085 : Radii of exoplanet host stars (van Belle+, 2009) J/A+A/501/297 : Effective temperatures of B Supergiants (Zorec+, 2009) J/ApJ/746/101 : Diameters and temperatures of AFG stars (Boyajian+, 2012) J/ApJ/757/112 : Stellar diameters. II. K and M-stars (Boyajian+, 2012) J/MNRAS/419/1637 : Nearby red clump stars JHK observations (Laney+, 2012) J/A+A/543/A160 : Normalized spectra of 82 Kepler red giants (Thygesen+, 2012) J/ApJ/771/40 : Main-sequence A, F, G & K stars photometry (Boyajian+, 2013) J/A+A/557/A70 : Evolved planet hosts - stellar parameters (Mortier+, 2013) J/A+A/554/A98 : Limb-darkening coefficients for red giants (Neilson+, 2013) J/ApJ/764/78 : Oxygen abundances in nearby FGK stars (Ramirez+, 2013) J/ApJ/775/45 : PTI carbon star angular size survey (van Belle+, 2013) J/ApJ/791/58 : C & O abund. across the Hertzsprung gap (Adamczak+, 2014) J/A+A/580/A24 : Abundances in dwarfs, subgiants & giants (da Silva+, 2015) J/A+A/574/A50 : Chemical abundances of giants and subgiants (Jofre+, 2015) J/AJ/150/88 : Abundances in the local region. I. G & K giants (Luck, 2015) J/A+A/588/A98 : Metallicities & abund. of evolved stars (Maldonado+, 2016) J/AJ/152/16 : Bolometric fluxes for cool evolved stars (van Belle+, 2016) J/A+A/599/A85 : Herbig AeBe disks at mas scale (Lazareff+, 2017) J/AJ/155/30 : Fundamental param. of 87 stars from the NPOI (Baines+, 2018) J/A+A/615/A31 : PTPS stars IV. (Deka-Szymankiewicz+, 2018) J/ApJS/240/21 : Symbiotic stars with 2MASS, WISE & Gaia data (Akras+, 2019) J/A+A/631/A108 : Disks around post-AGB binaries fit results (Kluska+, 2019) J/A+A/625/A141 : Abundances of disk and bulge giants (Lomaeva+, 2019) http://nexsci.caltech.edu/software/PTISupport/ : PTI support page Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Object Simbad name 11- 20 A10 --- SpT1 Primary literature/initial spectral type 22- 40 A19 --- r_SpT1 Reference/Source for SpT1 42- 53 A12 --- SpT2 Secondary literature/initial spectral type 55- 73 A19 --- r_SpT2 Reference/Source for SpT2 75- 79 I5 K Teff [2900/12000] Model Effective temperature 81- 83 F3.1 [cm/s2] logg [0.5/3] Model log surface gravity 85- 91 A7 --- SpT Our best fit spectral type 93- 98 F6.1 10-11W/m2 Flux [6.4/1130] Bolometric flux, 10-8erg/s/cm2 100- 103 F4.1 10-11W/m2 e_Flux [0.2/11.4] Uncertainty in Flux 105- 108 F4.1 % ErrFlux [0.6/11.4] Flux error (percentage) 110- 113 F4.2 mag Av [0/1.13] V-band reddening 115- 118 F4.2 mag e_Av [0/0.4] Uncertainty in Av 120- 123 F4.1 --- chi2/DoF [0.1/53] Fit χ2/DoF 125- 127 I3 --- DoF [1/155] Fit degrees of freedom -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Object Simbad name 11- 19 A9 --- Sys System/Wvlen 21- 24 A4 --- Band Band in System (or bandpass for Wvlen) 26- 28 A3 --- x_value Unit for value 30- 36 F7.2 --- value [-34.3/3882.7] Cataloged value 38- 44 F7.2 --- e_value [0/9378.1] Uncertainty in value 46- 64 A19 --- r_value Reference (bibcode) for value -------------------------------------------------------------------------------- Byte-by-byte Description of file: table9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Object Simbad name 11- 15 F5.3 mas SizeUD [0.79/8.3] Wavelength-specific uniform disk angular size 17- 21 F5.3 mas e_SizeUD [0.002/0.4] Uncertainty in UD 23- 27 F5.3 mas s_SizeUD [0.03/2.5] Systematic uncertainty in UD 29- 32 I4 K Teffi [3122/5223] Initial Effective Temperature, Table 17, Equation 1 34- 38 F5.3 --- UD2LD [1/1.1] SizeUD to LD correction 40- 44 F5.3 mas LD [0.8/8.51] Limb-darkened Rosseland mean angular diameter 46- 50 F5.3 mas e_LD [0.03/2.5] Uncertainty in LD 52- 55 F4.2 mag V0-K0 [1.9/8.6] Dereddened V-K color 57- 60 F4.2 mag e_V0-K0 [0.04/0.7] Uncertainty in V0-K0 62- 65 I4 K Teff [3033/5156] Computed Effective temperature 67- 69 I3 K e_Teff [29/679] Uncertainty in Teff -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Object Simbad name 11- 14 F4.2 mag V0-K0 [1.9/8.6] Dereddened V-K color 16- 19 F4.2 mag e_V0-K0 [0.04/0.7] Uncertainty in V0-K0 21- 28 A8 --- SpT Spectral Type 30- 34 F5.2 mas plx [0.89/96.54] Parallax, π 36- 39 F4.2 mas e_plx [0.03/0.9] Uncertainty in plx 41- 47 A7 --- r_plx Source for plx: Gaia DR2 or Hipparcos (HIP) 49- 54 F6.2 Rsun Rstar [7.66/303.12] Radius 56- 60 F5.2 Rsun e_Rstar [0.15/41.26] Uncertainty in Rstar 62- 68 F7.2 Lsun Lstar [28.52/7980.99] Luminosity 70- 76 F7.2 Lsun e_Lstar [0.44/2237.84] Uncertainty in Lstar -------------------------------------------------------------------------------- Byte-by-byte Description of file: table20.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Object Simbad name 11- 13 I3 --- NHp [1/670]? Number of H-band points 15- 19 F5.3 mas thetaH [0.6/3.5]? Angular diameter in H-band 21- 25 F5.3 mas e_thetaH [0.002/2]? Formal uncertainty in ThetaH 27- 31 F5.3 mas s_thetaH [0.028/0.3]? Systematic uncertainty in ThetaH 33- 35 I3 --- NK [2/701]? Number of K-band points 37- 41 F5.3 mas thetaK [0.79/4.8]? Angular diameter in K-band 43- 47 F5.3 mas e_thetaK [0.002/0.4]? Formal uncertainty in ThetaK 49- 53 F5.3 mas s_thetaK [0.04/0.375]? Systematic uncertainty in thetaK 55- 59 F5.3 mas AvgRes [0/0.17] Average residual of the ThetaK fit 61- 64 F4.2 --- chi2/DoF [0.05/4.8]? Fit χ2/DoF -------------------------------------------------------------------------------- Byte-by-byte Description of file: table21.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Object Simbad name 10- 13 F4.2 [cm/s2] logg [0.3/3.3] Reported log(g) value (cgs) 15- 18 F4.2 [cm/s2] e_logg [0.04/0.5]? Uncertainty in logg (1) 20- 38 A19 --- r_logg Reference (bibcode) for logg 40- 45 F6.2 Rsun Rstar [7.6/196] Radius 47- 51 F5.2 Rsun e_Rstar [0.15/14] Uncertainty in Rstar 53- 57 F5.2 Msun Mstar [0.5/36.1] Derived Mass 59- 63 F5.2 Msun e_Mstar [0.1/22] Uncertainty in Mstar (1) 65- 65 A1 --- u_Mstar Uncertainty flag on Mstar (1) -------------------------------------------------------------------------------- Note (1): For references that did not report a formal error in log(g), a value of 0.25dex was assumed and the resulting error in M is flagged (u_Mstar=:). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 27-Mar-2023
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