UCAC2 40854773 , the SIMBAD biblio

2018ApJ...869..122L - Astrophys. J., 869, 122-122 (2018/December-3)

GD-1: the relic of an old metal-poor globular cluster.

LI G.-W., YANNY B. and WU Y.

Abstract (from CDS):

Combining data from Gaia DR2, SDSS DR14, and LAMOST DR6, we update the fit to model of the properties of the stellar stream GD-1 and find that it has an age of ∼13 Gyr, [Fe/H] of -2.2 ± 0.12, and a distance from the Sun of ∼8 kpc. We tabulate six-dimensional (6D) phase-space fiducial points along the GD-1 stream orbit over a 90° arc. The fitted orbit shows that the stream has an eccentricity e ∼ 0.3, perigalacticon of 14.2 kpc, apogalacticon of 27.0 kpc, and inclination i ∼ 40°. There is evidence along the arc for four candidate stellar overdensities, one candidate gap, two candidate stellar underdensities, and that the stream is cut off at ph1 ∼ 2° (in the stream-aligned (ph1, ph2) coordinate system of Koposov et al.). The spur originating at ph1 ∼ -40° implies stars were pulled away from the stream trace by an encounter (potentially a dark matter subhalo). The narrowest place (FWHM ∼ 44.6 pc) of the GD-1 trace is at (ph1, ph2c) ∼ (-14°, 0.°15), which is ∼(178.°18, 52.°19) in (R.A., decl.), where the progenitor is possibly located. We also find six blue horizontal branch and 10 blue stragglers spectroscopic stars in the GD-1 stream.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): Galaxy: abundances - Galaxy: kinematics and dynamics - Galaxy: structure - globular clusters: general

VizieR on-line data: <Available at CDS (J/ApJ/869/122): table3.dat table4.dat table6.dat table7.dat table8.dat>

Simbad objects: 160

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