A Dust Lane Leading the Galactic Bar at Negative Galactic Longitudes
Open Access
- 20 January 1996
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 457 (1), L27
- https://doi.org/10.1086/309885
Abstract
Comparing the different wavelengths of the DIRBE integrated surface brightness maps at positive and negative Galactic longitudes on the plane near the Galactic center, it is shown that there exists a thick dust lane (between 1.0 and 2.6 mag of absorption in K) at negative longitudes (as compared to positive ones), which follows the "standard" interstellar extinction law. A likely explanation for this effect is the existence of a thick dust lane preceding the bar. This will have to be confirmed by future infrared surveys, such as DENIS or 2MASS, that will cover negative Galactic longitudes, where a heavy extinction dust lane about 2° wide, close to the Galactic plane, should be seen.Keywords
This publication has 8 references indexed in Scilit:
- Intrinsic Bar/Ring Misalignment and a Starburst Nuclear Ring in the Peculiar Spiral Galaxy ESO 565-11The Astronomical Journal, 1995
- Morphology, near-infrared luminosity, and mass of the Galactic bulge from COBE DIRBE observationsThe Astrophysical Journal, 1995
- Infrared signatures of the inner spiral arms and barMonthly Notices of the Royal Astronomical Society, 1994
- A two-micron Galactic surveyMonthly Notices of the Royal Astronomical Society, 1993
- The centre of the Milky WayNature, 1993
- Detection of a large-scale stellar bar in the Milky WayThe Astrophysical Journal, 1992
- Understanding the kinematics of Galactic Centre gasMonthly Notices of the Royal Astronomical Society, 1991
- Interstellar Dust and ExtinctionAnnual Review of Astronomy and Astrophysics, 1990