100 μm and 160 μm emission as resolved star-formation rate estimators in M 33 (HERM33ES)

MLA

E. M. Xilouris, et al. 100 Μm and 160 Μm Emission as Resolved Star-Formation Rate Estimators in M 33 (HERM33ES). July 2010. EBSCOhost, https://doi.org/10.1051/0004-6361/201014649⟩.

APA

E. M. Xilouris, F. F. S. van der Tak, B. S. Koribalski, Fatemeh Tabatabaei, J. Braine, Frank P. Israel, S. Verley, Francoise Combes, Markus Röllig, D. Calzetti, P. van der Werf, M. Boquien, C. Kramer, G. Quintana-Lacaci, Monica Relaño, Remo P. J. Tilanus, S. D. Lord, Gordon J. Stacey, Christof Buchbender, & Frank Bertoldi. (2010). 100 μm and 160 μm emission as resolved star-formation rate estimators in M 33 (HERM33ES). https://doi.org/10.1051/0004-6361/201014649⟩

Chicago

E. M. Xilouris, F. F. S. van der Tak, B. S. Koribalski, Fatemeh Tabatabaei, J. Braine, Frank P. Israel, S. Verley, et al. 2010. “100 Μm and 160 Μm Emission as Resolved Star-Formation Rate Estimators in M 33 (HERM33ES),” July. doi:10.1051/0004-6361/201014649⟩.