2001ApJ...548L.165O


Query : 2001ApJ...548L.165O

2001ApJ...548L.165O - Astrophys. J., 548, L165-L169 (2001/February-3)

Detection of massive tidal tails around the globular cluster Palomar 5 with Sloan Digital Sky Survey commissioning data.

ODENKIRCHEN M., GREBEL E.K., ROCKOSI C.M., DEHNEN W., IBATA R., RIX H.-W., STOLTE A., WOLF C., ANDERSON J.E.Jr, BAHCALL N.A., BRINKMANN J., CSABAI I., HENNESSY G., HINDSLEY R.B., IVEZIC Z., LUPTON R.H., MUNN J.A., PIER J.R., STOUGHTON C. and YORK D.G.

Abstract (from CDS):

We report the discovery of two well-defined tidal tails emerging from the sparse remote globular cluster Palomar 5. These tails stretch out symmetrically to both sides of the cluster in the direction of constant Galactic latitude and subtend an angle of 2°.6 on the sky. The tails have been detected in commissioning data of the Sloan Digital Sky Survey, providing deep five-color photometry in a 2°.5-wide band along the equator. The stars in the tails make up a substantial part (~(1)/(3)) of the current total population of cluster stars in the magnitude interval 19.5≤i*≤22.0. This reveals that the cluster is subject to heavy mass loss. The orientation of the tails provides an important key for the determination of the cluster's Galactic orbit.

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Journal keyword(s): Galaxy: Halo - Galaxy: Kinematics and Dynamics - Galaxy: Structure - Galaxy: Globular Clusters:: Individual Name: Palomar 5

Nomenclature: NAME Palomar 5 Stream N=1.

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 ACO 2035 ClG 15 12 08 -06 03.2           ~ 8 0
2 NAME Palomar 5 Stream St* 15 16 05 -00 06.7           ~ 132 0
3 Cl Pal 5 GlC 15 16 05.30 -00 06 41.0   15.1       ~ 797 1
4 ACO 2050 ClG 15 16 18.7 +00 05 31           ~ 122 0

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