GD-1: The Relic of an Old Metal-poor Globular Cluster
Journal Article
·
· The Astrophysical Journal (Online)
- Chinese Academy of Sciences (CAS), Beijing (China)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Combining data from Gaia DR2, SDSS DR14 and LAMOST DR6, we update the fit tomodel of the properties of the stellar stream GD-1 and find that it has an ageof $$\sim 13$$ Gyr, [Fe/H] of $$-2.2\pm 0.12$$, and a distance from the sun of $$\sim 8$$ kpc. We tabulate 6D phase-space fiducial points along the GD-1 streamorbit over a 90$$^\circ$$ arc. The fitted orbit shows that the stream has aneccentricity $$e \sim 0.3$$, perigalacticon of 14.2 kpc, apogalacticon of 27.0 kpc and inclination $$i \sim 40^{\circ}$$. There is evidence along the arc for 4candidate stellar overdensities, one candidate gap, two candidate stellarunderdensities and is cut off at $$\phi_1 \sim 2^{\circ}$$ (in the stream-aligned$$(\phi_1,\phi_2)$$ coordinate system. The spur originating at $$\phi_1 \sim -40^{\circ}$$ implies stars were pulled away from the stream traceby an encounter (potentially a dark matter subhalo). The narrowest place ( FWHM$$\sim 44.6$$ pc) of the GD-1 trace is at $$(\phi_1, \phi_2^c) \sim (-14^{\circ},0.15^{\circ})$$, which is $$\sim (178.18^{\circ}, 52.19^{\circ})$$ in (R. A.,Decl.), where the progenitor is possibly located. In conclusion, we also find six BHB and 10BS spectroscopic stars in the GD-1 stream.
- Research Organization:
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
- Grant/Contract Number:
- AC02-07CH11359
- OSTI ID:
- 1498554
- Report Number(s):
- FERMILAB-PUB--18-746-CD; arXiv:1811.06427; 1722223
- Journal Information:
- The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 869; ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Formation Imprints in the Kinematics of the Milky Way Globular Cluster System
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journal | September 2019 |
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