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Query : 2012A&A...546L...7M |
2012A&A...546L...7M - Astronomy and Astrophysics, volume 546, L7-7 (2012/10-1)
Clumpy streams in a smooth dark halo: the case of Palomar 5.
MASTROBUONO-BATTISTI A., DI MATTEO P., MONTUORI M. and HAYWOOD M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Galaxy: halo - globular clusters: individual: Palomar 5 - Galaxy: evolution - Galaxy: kinematics and dynamics - methods: numerical
Simbad objects: 5
Number of rows : 5 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2023 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | NAME Gal Anticenter | reg | 05 46 | +28.9 | ~ | 853 | 0 | |||||
2 | NGC 5466 | GlC | 14 05 27.29 | +28 32 04.0 | 9.70 | ~ | 809 | 0 | ||||
3 | NAME Serpens Dwarf | GlC | 15 16 05.30 | -00 06 41.0 | 15.1 | ~ | 711 | 1 | ||||
4 | NAME Galactic Center | reg | 17 45 39.60213 | -29 00 22.0000 | ~ | 13679 | 0 | |||||
5 | NAME GD-1 Stream | St* | ~ | ~ | ~ | 234 | 0 |
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