Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-02-03
Astrophys.J. 621 (2005) L105-L108
Astronomy and Astrophysics
Astrophysics
8 pages, 4 figures. accepted by ApJL
Scientific paper
10.1086/429291
We present the result of a near-infrared (J H Ks) survey along the Galactic plane, -10.5deg < l < +10.5deg and b=+1.0deg, with the IRSF 1.4m telescope and the SIRIUS camera. Ks vs. H-Ks color-magnitude diagrams reveal a well-defined population of red clump (RC) stars whose apparent magnitude peak changes continuously along the Galactic plane, from Ks=13.4 at l=-10deg to Ks=12.2 at l=+10deg after dereddening. This variation can be explained by the bar-like structure found in previous studies, but we find an additional inner structure at |l| < 4deg, where the longitude - apparent magnitude relation is distinct from the outer bar, and the apparent magnitude peak changes by only 0.1 mag over the central 8deg. The exact nature of this inner structure is as yet uncertain.
Baba Daisuke
Haba Yasuaki
Kadowaki Ryota
Kato Daisuke
Kurita Mikio
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