Attenuation Curves in Clumpy, Galactic Envrionments
- Data will be available soon.
- http://arxiv.org/abs/1606.02030
MoCafe/Galaxy
- The current version of MoCafe/Galaxy is publicly available here.
- The code runs in parallel using openmp/mpi and is being updated and tested to include the infrared emission and polarization. (The published code is only for scattering.)
- More complete description will be published in a forthcoming paper.
- References:
- Shinn & Seon (2015, ApJ)
- Lee et al. (2015, ApJ, 806,274)
- Seon (2015, JKAS, 48, 57)
- Seon et al. (2014, ApJ, 785, L18)
- Choi et al. (2013, ApJ, 774, 34)
- Lim et al. (2013, ApJ, 765, 107)
- Seon & Witt (2012, ApJ, 758, 109)
- Jo et al. (2012, ApJ, 756,38)
- Seon (2009, ApJ, 703, 1159)
- Lee et al. (2008, ApJ, 686, 1155)