E. Nelson, P. van Dokkum, N. Schreiber, M. Franx, G. Brammer, I. Momcheva, S. Wuyts, K. Whitaker, R. Skelton, M. Fumagalli and 10 other author(s). (2015)cite arxiv:1507.03999Comment: Submitted to ApJ. Main results: Fig. 6 shows the scale lengths of ionized gas vs. stellar disks. Fig. 9 shows where Halpha in galaxies is enhanced above and suppressed below the star-forming main sequence. Data points for Halpha profiles are available upon request.
M. Cerviño. (2013)cite arxiv:1312.0015Comment: Published in New Astronomy Reviews; Vol 57, p 123 (2013) 18 pags, 11 Figures (best quality figures in the journal version).
S. Offner, P. Clark, P. Hennebelle, N. Bastian, M. Bate, P. Hopkins, E. Moraux, and A. Whitworth. (2013)cite arxiv:1312.5326Comment: 24 pages, 6 figures. Accepted for publication as a chapter in Protostars and Planets VI, University of Arizona Press (2014), eds. H. Beuther, R. S. Klessen, C. P. Dullemond, Th. Henning.
C. Li, R. de Grijs, and L. Deng. (2014)cite arxiv:1412.5368Comment: 9 pages, 5 figures, Äuthors' version of a letter published in Nature (17 December 2014), including Methods and Extended Data.".