no code implementations • 26 Feb 2021 • N. Falstad, S. Aalto, S. König, K. Onishi, S. Muller, M. Gorski, M. Sato, F. Stanley, F. Combes, E. González-Alfonso, J. G. Mangum, A. S. Evans, L. Barcos-Muñoz, G. C. Privon, S. T. Linden, T. Díaz-Santos, S. Martín, K. Sakamoto, N. Harada, G. A. Fuller, J. S. Gallagher, P. P. van der Werf, S. Viti, T. R. Greve, S. García-Burillo, C. Henkel, M. Imanishi, T. Izumi, Y. Nishimura, C. Ricci, S. Mühle
We find no dependence on the inclination of the host galaxy, but strong evidence of lower IRAS 25 to 60 {\mu}m flux density ratios (f25/f60) in CONs compared to the rest of the sample.
Astrophysics of Galaxies
no code implementations • 1 Mar 2019 • C. Yang, R. Gavazzi, A. Beelen, P. Cox, A. Omont, M. D. Lehnert, Y. Gao, R. J. Ivison, A. M. Swinbank, L. Barcos-Muñoz, R. Neri, A. Cooray, S. Dye, S. Eales, H. Fu, E. González-Alfonso, E. Ibar, M. J. Michałowski, H. Nayyeri, M. Negrello, J. Nightingale, I. Pérez-Fournon, D. A. Riechers, I. Smail, P. van der Werf
The reconstructed dust emission in the source plane is dominated by a compact disk with an effective radius of 0. 7kpc plus an overlapping extended disk with a radius twice as large.
Astrophysics of Galaxies