Grain size limits derived from 3.6 mu m and 4.5 mu m coreshine



: Steinacker J, Andersen M, Thi WF, Paladini R, Juvela M, Bacmann A, Pelkonen VM, Pagani L, LefSvre C, Henning T, Noriega-Crespo A

Publisher: EDP SCIENCES S A

: 2015

 Astronomy and Astrophysics

: ASTRONOMY & ASTROPHYSICS

: ASTRON ASTROPHYS

: ARTN A70

: 582

: 23

: 1432-0746

DOI: https://doi.org/10.1051/0004-6361/201425434


Conclusions. Considering surface brightness ratios in the 3.6 and 4.5 mu m bands across a molecular cloud core is an effective method of disentangling the complex interplay of structure and opacities when used in combination with observed limits of the optical depth.




Last updated on 26/11/2024 10:32:58 AM