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Autor:
Audcent-Ross, Fiona M, Meurer, Gerhardt R, Wong, OI, Zheng, Z, Hanish, D, Zwaan, MA, Bland-Hawthorn, J, Elagali, A, Meyer, M, Putman, ME, Ryan-Webber, EV, Sweet, SM, Thilker, DA, Seibert, M, Allen, R, Dopita, MA, Doyle-Pegg, MT, Drinkwater, M, Ferguson, HC, Freeman, KC, Heckman, TM, Jr, RC Kennicutt, Kilborn, VA, Kim, JH, Knezek, PM, Koribalski, B, Smith, RC, Staveley-Smith, L, Webster, RL, Werk, JK
For the first time both H$\alpha$ and far-ultraviolet (FUV) observations from an HI-selected sample are used to determine the dust-corrected star formation rate density (SFRD: $\dot{\rho}$) in the local Universe. Applying the two star formation rate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8698932fc465b2f43cf8167171e5358
https://www.repository.cam.ac.uk/handle/1810/282915
https://www.repository.cam.ac.uk/handle/1810/282915
