J/ApJ/907/10   Initial vs final sample of the VMP HK/HES stars  (Limberg+, 2021)

Dynamically Tagged Groups of Very Metal-poor Halo Stars from the HK and Hamburg/ESO Surveys. Limberg G., Rossi S., Beers T.C., Perottoni H.D., Perez-Villegas A., Santucci R.M., Abuchaim Y., Placco V.M., Lee Y.S., Christlieb N., Norris J.E., Bessell M.S., Ryan S.G., Wilhelm R., Rhee J., Frebel A. <Astrophys. J., 907, 10 (2021)> =2021ApJ...907...10L 2021ApJ...907...10L
ADC_Keywords: Stars, metal-deficient; Spectra, optical; Abundances, [Fe/H]; Effective temperatures; Radial velocities; Proper motions Keywords: Milky Way dynamics ; Milky Way evolution ; R-process ; Population II stars ; Milky Way stellar halo Abstract: We analyze the dynamical properties of ∼1500 very metal-poor (VMP; [Fe/H]≲-2.0) halo stars, based primarily on medium-resolution spectroscopic data from the HK and Hamburg/ESO surveys. These data, collected over the past 30yr, are supplemented by a number of calibration stars and other small samples, along with astrometric information from Gaia DR2. We apply a clustering algorithm to the 4D energy-action space of the sample, and identify a set of 38 dynamically tagged groups (DTGs), containing between 5 and 30 member stars. Many of these DTGs can be associated with previously known prominent substructures such as Gaia-Sausage/Enceladus (GSE), Sequoia, Helmi Stream (HStr), and Thamnos. Others are associated with previously identified smaller dynamical groups of stars and streams. We identify 10 new DTGs as well, many of which have strongly retrograde orbits. We also investigate possible connections between our DTGs and ∼300 individual r-process-enhanced (RPE) stars from a recent literature compilation. We find that several of these objects have similar dynamical properties to GSE (5), the HStr (4), Sequoia (1), and Rg5 (1), indicating that their progenitors might have been important sources of RPE stars in the Galaxy. Additionally, a number of our newly identified DTGs are shown to be associated with at least two RPE stars each (DTG-2:3, DTG-7:2; DTG-27:2). Taken as a whole, these results are consistent with ultra-faint and/or dwarf spheroidal galaxies as birth environments in which r-process nucleosynthesis took place, and then were disrupted by the Milky Way. Description: In this work, we have considered the dynamical properties of the very metal poor (VMP; [Fe/H]≲-2.0) stars primarily selected from the HK/HES surveys. Over the past three decades, the metal-poor candidates identified in these surveys have been followed-up with medium-resolution (1200≲R∼2000) spectroscopy with a wide variety of telescopes and instruments. The typical spectral coverage of these spectra are 3500-5000Å, although there was wide variation. The decisions as to which targets to observe are difficult to quantify, since many observers contributed to these efforts. In addition, in some cases, photometric information from independent efforts (HK), or taken directly from an approximate calibration of the prism spectra (HES), were obtained in advance of the spectroscopic follow-up. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 125 4443 Initial sample of the VMP HK/HES stars table6.dat 115 1526 Final sample of the VMP HK/HES stars -------------------------------------------------------------------------------- See also: I/337 : Gaia DR1 (Gaia Collaboration, 2016) I/345 : Gaia DR2 (Gaia Collaboration, 2018) I/349 : StarHorse, Gaia DR2 photo-astrometric distances (Anders+, 2019) VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006) J/AJ/90/2089 : Stars of very low metal abundance. I (Beers+, 1985) J/ApJS/61/667 : Kinematics of Galactic old population (Norris 1986) J/AJ/103/1987 : Stars of very low metal abundance (Beers+ 1992) J/AJ/117/981 : Estimation of stellar metal abundance. II. (Beers+, 1999) J/MNRAS/320/451 : A-G star metallicity (Beers+, 2001) J/A+A/416/1117 : Abundances in the early Galaxy (Cayrel+, 2004) J/AJ/130/2804 : Carbon abundances in metal-poor stars (Rossi+, 2005) J/ApJ/652/1585 : Bright metal-poor stars from HES survey (Frebel+, 2006) J/ApJ/655/492 : Equivalent widths of 26 metal-poor stars (Aoki+, 2007) J/A+A/484/721 : HES survey. IV. Candidate metal-poor stars (Christlieb+, 2008) J/AJ/136/2050 : SEGUE stellar parameter pipeline. II. (Lee+, 2008) J/ApJ/703/2177 : Metal-poor MS turnoff stars summary (Schlaufman+, 2009) J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009) J/ApJ/719/931 : Chemical evolution of the UMi dSph (Cohen+, 2010) J/ApJ/714/663 : Stellar density map of the Milky Way (de Jong+, 2010) J/A+A/511/L10 : Abundances and space velocities of 94 stars (Nissen+, 2010) J/AJ/139/1051 : Carbon-enhanced metal-poor stars in the Galaxy (Placco+, 2010) J/ApJ/711/573 : Detailed abundances in a halo stellar stream (Roederer+, 2010) J/AJ/141/90 : SEGUE stellar parameter pipeline. V. (Lee+, 2011) J/AJ/142/188 : Metal-poor stars from the HES using CH G-band (Placco+, 2011) J/ApJ/749/77 : MW halo. III. Statistical chemic abundances (Schlaufman+, 2012) J/ApJ/794/58 : Metal-poor stars in the thick disk of the Galaxy (Beers+, 2014) J/ApJ/788/180 : Very metal-poor stars in the Milky Way's halo (Carollo+, 2014) J/ApJ/781/40 : Metal-poor stars HES survey. II. Spectroscopy (Placco+, 2014) J/ApJ/797/21 : Carbon-enhanced metal-poor stars (Placco+, 2014) J/AJ/147/136 : Stars of very low metal abundance. VI. Abund. (Roederer+, 2014) J/MNRAS/448/822 : LAMOST candidate members of star clusters (Xiang+, 2015) J/AJ/151/82 : 4 brightest red giants in the UFD galaxy Ret2 (Roederer+, 2016) J/ApJ/835/81 : Bright metal-poor stars from HES Survey. II. (Beers+, 2017) J/ApJ/838/44 : Abundances of the brightest member of Tuc III (Hansen+, 2017) J/A+A/618/A93 : Gaia DR2 open clusters in the Milky Way (Cantat-Gaudin+, 2018) J/A+A/616/A10 : 46 open clusters GaiaDR2 HR diagrams (Gaia Collaboration, 2018) J/A+A/616/A12 : Gaia DR2 sources in GC and dSph (Gaia Collaboration+, 2018) J/ApJ/858/92 : RPA Southern Pilot Search of 107 Stars (Hansen+, 2018) J/ApJ/852/49 : Properties of metal-poor stars in APOGEE DR13 (Hayes+, 2018) J/ApJS/238/16 : LAMOST-DR3 very metal-poor star catalog (Li+, 2018) J/AJ/155/256 : Spectroscopic validation RAVE metal-poor stars (Placco+, 2018) J/AJ/156/179 : Highly r-process-enhanced stars kinematics (Roederer+, 2018) J/ApJ/868/110 : R-Process Alliance 1st release in Galactic halo (Sakari+, 2018) J/A+A/623/A128 : Galactic halo CEMP stars abund. & kinematics (Hansen+, 2019) J/ApJ/882/177 : Abundances of 4 member stars of Tucana III (Marshall+, 2019) J/ApJ/870/122 : Spectroscopy of low-metallicity star candidates (Placco+, 2019) J/ApJ/894/34 : Metallicity gradient SDSS & SMSS in halo stars (Dietz+, 2020) J/ApJ/898/150 : High-res. MIKE obs. of metal-poor stars (Ezzeddine+, 2020) J/ApJS/249/30 : R-Process Alliance metal-poor star spectro. (Holmbeck+, 2020) J/A+A/638/A76 : StarHorse data for 5 surveys (Queiroz+, 2020) J/ApJ/891/39 : LAMOST DR3 very metal-poor stars of Galactic halo (Yuan+, 2020) Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- 2MASS 2MASS identifier 18- 30 A13 --- HK HK survey identifier 32- 44 A13 --- HES Hamburg/ESO survey identifier 46- 66 A21 --- OName Other identifier 68- 75 F8.4 deg RAdeg [0.003/360] Right Ascension in decimal degrees (J2000) 77- 84 F8.4 deg DEdeg [-86/75] Declination in decimal degrees (J2000) 86- 89 F4.1 mag Vmag [5.7/21.1]? Apparent V band magnitude 91- 94 I4 K Teff [4010/6998] Effective temperature 96- 99 F4.2 [cm/s2] logg [0.12/5] log surface gravity 101-105 F5.2 [Sun] [Fe/H] [-4.61/-1.8] Metallicity 107 A1 --- f_[Fe/H] [d] Flag on [Fe/H] (1) 109 A1 --- l_[C/Fe] Limit flag on [C/Fe] 110-114 F5.2 [Sun] [C/Fe] [-2.27/4.92]? log C/Fe abundance 116 A1 --- f_[C/Fe] [d] Flag on [C/Fe] (1) 118 A1 --- l_[C/Fe]c Limit flag on [C/Fe]c 119-123 F5.2 [Sun] [C/Fe]c [-2.27/4.92]? log corrected C/Fe abundance (2) 125 A1 --- f_[C/Fe]c [d] Flag on [C/Fe]c (1) -------------------------------------------------------------------------------- Note (1): Flag as follows: d = CEMP star with Teff≤4500K. The [Fe/H], [C/Fe], and [C/Fe]c ratios should be taken with caution (Section A.1). Note (2): Corrected for their evolutionary status (Placco+, 2014, J/ApJ/797/21). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- 2MASS 2MASS identifier 18- 21 I4 km/s RVel [-519/524] Radial velocity (1) 23- 28 F6.1 km/s RVelG [-397/492]? Gaia DR2 radial velocity 30- 34 F5.2 kpc Dist [0.03/17.4] StarHorse distance (2) 36- 39 F4.2 kpc e_Dist [0.0/3.32] Uncertainty in Dist 41- 48 F8.2 mas/yr pmRA [-1115/936] Gaia DR2 proper motion in RA 50- 57 F8.2 mas/yr pmDE [-1836/516] Gaia DR2 proper motion in DE 59- 63 F5.2 10+5km2/s2 E [-2.03/-0.16] Energy 65- 69 F5.2 10+3kpc.km/s JR [0.01/44.4] Radial action 71- 75 F5.2 10+3kpc.km/s Jth [-3.76/4.17] Azimuthal action 77- 80 F4.2 10+3kpc.km/s Jz [0/4.82] Vertical action 82- 85 F4.2 --- e [0.08/0.99] Eccentricity 87- 91 F5.1 deg i [1.6/179] Inclination 93- 99 F7.2 km/s RV [-484/416] Radial velocity 101-107 F7.2 km/s vth [-472/500] Azimuthal velocity 109-115 F7.2 km/s vz [-451/550] Vertical velocity -------------------------------------------------------------------------------- Note (1): From the medium-resolution spectroscopy (corrected to the heliocentric frame). Note (2): From Anders+, 2019, I/349, as described in Section 2.3. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 30-May-2022
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