Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S298(9), p. 423-423, 2013
DOI: 10.1017/s1743921313006893
Full text: Unavailable
AbstractWe estimate the 3D extinction law in the optical–NIR bands for a line of sight in the 2nd quadrant of the Galactic disk. Two dust lanes are identified at ~9 and ~10.25 kpc in both AV and RV, indicating that the size of the dust grains in the spiral arms is larger than that in the inter-arm regions.