Volume 439, Number 2, August IV 2005
|Page(s)||L5 - L8|
|Published online||29 July 2005|
Letter to the Editor
Searching for merger debris in the Galactic halo: chemodynamical evidence based on local blue HB stars
Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Correo Central, Santiago, Chile e-mail: firstname.lastname@example.org
2 Pontificia Universidad Católica de Chile, Departamento de Astronomía y Astrofísica, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile e-mail: [mcatelan;mzoccali]@astro.puc.cl
Accepted: 26 June 2005
We report on the discovery of a group of local A-type blue horizontal-branch (HBA) stars moving in a prograde, comet-like orbit with very similar kinematics and abundances. This serendipitously discovered group contains 5 or 6 local HBA stars venturing very close to the Galactic centre; their [Fe/H] is around -1.7, and they seem to present minimum scatter in at least Mg, Si, Ti, Fe, Al, and Cr abundances. This “Cometary Orbit Group” (COG) was found while we were testing a new method to detect the debris associated with the merger of smaller, specific protogalactic entities into our galaxy. The method is primarily intended to identify field HBA stars with similar kinematics and detailed, multi-species abundance patterns as seen among members of a surviving remnant (e.g., ω Centauri). Quite possibly, the COG is the remnant, on a highly decayed orbit, of a merging event that took place in the relatively remote past (i.e., at least one revolution ago).
Key words: astrometry / stars: kinematics / stars: horizontal branch / Galaxy: halo / Galaxy: structure
© ESO, 2005
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