Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100 pc scales in M 51

Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100 pc scales in M 51DOI: info:10.1051/0004-6361/201834915v. 625A19
Querejeta, M., Schinnerer, E., Schruba, A., Murphy, E., Meidt, S., Usero, A., Leroy, A. K., Pety, J., Bigiel, F., Chevance, M., Faesi, C. M., Gallagher, M., García-Burillo, S., Glover, S. C. O., Hygate, A. P. S., Jiménez-Donaire, M. J., Kruijssen, J. M. D., Momjian, E., Rosolowsky, E., and Utomo, D. 2019. "Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100 pc scales in M 51." Astronomy and Astrophysics, 625 A19. https://doi.org/10.1051/0004-6361/201834915.
ID: 151827
Type: article
Keywords: SAO