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A Distinct Structure inside the Galactic Bar
Author(s) -
Shogo Nishiyama,
Tetsuya Nagata,
Daisuke Baba,
Y. Haba,
Ryota Kadowaki,
Daisuke Kato,
Mikio Kurita,
Chie Nagashima,
Takahiro Nagayama,
Yuka Murai,
Yasushi Nakajima,
Motohide Tamura,
Hidehiko Nakaya,
Koji Sugitani,
Takahiro Naoi,
Noriyuki Matsunaga,
Toshihiko Tanabé,
Nobuhiko Kusakabe,
Shuji Sato
Publication year - 2005
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/429291
Subject(s) - magnitude (astronomy) , physics , astrophysics , sirius , galactic plane , stars , absolute magnitude , bar (unit) , longitude , population , astronomy , latitude , demography , sociology , meteorology
We present the result of a near-infrared (J H Ks) survey along the Galacticplane, -10.5deg < l < +10.5deg and b=+1.0deg, with the IRSF 1.4m telescope andthe SIRIUS camera. Ks vs. H-Ks color-magnitude diagrams reveal a well-definedpopulation of red clump (RC) stars whose apparent magnitude peak changescontinuously along the Galactic plane, from Ks=13.4 at l=-10deg to Ks=12.2 atl=+10deg after dereddening. This variation can be explained by the bar-likestructure found in previous studies, but we find an additional inner structureat |l| < 4deg, where the longitude - apparent magnitude relation is distinctfrom the outer bar, and the apparent magnitude peak changes by only 0.1 magover the central 8deg. The exact nature of this inner structure is as yetuncertain.Comment: 8 pages, 4 figures. accepted by ApJ

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