Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-09-09
Mon.Not.Roy.Astron.Soc. 338 (2003) 253
Astronomy and Astrophysics
Astrophysics
accepted to MNRAS, 12 pages and 14 figures
Scientific paper
10.1046/j.1365-8711.2003.06049.x
We extract J and K_s magnitudes from the 2MASS Point Source Catalog for approximately 6 million stars with 8 < K_s < 13 in order to build an A_K extinction map within 10 degrees of the Galactic centre. The extinction was determined by fitting the upper giant branch of (K_s, J-K_s) colour-magnitude diagrams to a dereddened upper giant branch mean locus built from previously studied Bulge fields. The extinction values vary from A_K=0.05 in the edges of the map up to A_K=3.2 close to the Galactic centre. The 2MASS extinction map was compared to that recently derived from DENIS data. Both maps agree very well up to A_K=1.0. The 2MASS extinction values were also compared to those obtained from dust emission in the far infrared using DIRBE/IRAS. Several systematic effects likely to bias this comparison were addressed, including the presence of dust on the background of the bulk of 2MASS stars used in the extinction determination. For the region with $3^{\circ}<|b|<5^{\circ}$, where the dust contribution on the far side of the Galaxy is $\approx$ 5%, the two extinction determinations correlate well, but the dust emission A_K values are systematically higher than those from 2MASS. A calibration correction factor of 76% for the DIRBE/IRAS dust emission extinction is needed to eliminate this systematic effect. Similar comparisons were also carried out for the $1^{\circ}<|b|<3^{\circ}$ and $|b| < 0.5^{\circ}$ strips. An asymmetry relative to the Galactic plane is observed in the dust maps, roughly in the sense that A_K values are 60% smaller in the south than in the north for $1^{\circ}<|b|<5^{\circ}$. This asymmetry is due to the presence of foreground dust clouds mostly in the northern region of the Bulge.
Barbuy Batriz
Bica Eduardo L. D.
Dutra Carlos M.
Santiago Basilio X.
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