Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Alyssa D. Sokol"'
UV-FIR SED modeling is an effective way to disentangle emission between star formation (SF) and active galactic nuclei (AGN) in galaxies; however, this approach becomes uncertain for composite AGN/SF galaxies that comprise 50-70% of IR-samples. Cosmi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4acabc8292b0b460a8b3295bd4f16507
http://arxiv.org/abs/2302.10374
http://arxiv.org/abs/2302.10374
Autor:
Michael M. Dunham, Thomas Henning, Mark H. Heyer, John J. Tobin, Scott J. Wolk, Robert A. Gutermuth, William J. Fischer, Judith L. Pipher, Joseph L. Hora, Riwaj Pokhrel, Stella S. R. Offner, Alyssa D. Sokol, Thomas Allen, S. K. Betti, Lori Allen, S. Thomas Megeath, Babar Ali, Philip C. Myers
Publikováno v:
The Astrophysical Journal. 896:60
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::18e982d93bdbab25d9465d1e182e080e
https://doi.org/10.3847/1538-4357/ab92a2
https://doi.org/10.3847/1538-4357/ab92a2
