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A&A 456, 905-910 (2006)
DOI: 10.1051/0004-6361:20065507
Carbon stars in the outer spheroid of NGC 6822
S. Demers1, P. Battinelli2 and E. Artigau11 Département de Physique, Université de Montréal, CP 6128, Succursale Centre-Ville, Montréal, Qc, H3C 3J7, Canada
e-mail: [demers;artigau]@astro.umontreal.ca
2 INAF, Osservatorio Astronomico di Roma Viale del Parco Mellini 84, 00136 Roma, Italy
e-mail: battinel@oarhp1.rm.astro.it
(Received 26 April 2006 / Accepted 12 June 2006)
Abstract
Context.From a 2
2° of NGC 6822 survey we have previously
established that this
Local Group dwarf irregular galaxy possesses a huge spheroid
having more than one degree in length. This spheroid is in rotation
but its rotation curve is known only within ~15' from the center.
It is therefore critical to identify bright stars belonging to the spheroid
to characterize,
as far as possible, its outer kinematics.
Aims.We use the new wide field near infrared imager CPAPIR, operated by the SMARTS
consortium, to acquire
J,
images of two
areas in the outer spheroid to
search for C stars.
Methods.The colour diagram of the fields allows the identification of 192
C stars candidates but a study of the FWHM of the images permits the
rejection of numerous non-stellar objects with colours similar to C stars.
Results. We are left with 75 new C stars, their mean
magnitude and mean
colour are similar to the bulk of known NGC 6822 C stars.
Conclusions.This outer spheroid survey confirms that the intermediate-age AGB stars are
a major contributor to the stellar populations of the spheroid. The discovery
of some 50 C stars well beyond the limit of the previously known rotation curve
calls for a promising spectroscopic follow-up to a major axis distance of 40'.
Key words: galaxies: individual: NGC 6822 -- galaxies: structure -- stars: carbon -- galaxies: dwarf
© ESO 2006
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