Autor der Publikation

Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4

, , , , , , , , und . (2015)cite arxiv:1511.04443Comment: Submitted to ApJ Letters. Fig. 2. shows measured radial Balmer decrement profiles. Fig. 3 shows inferred dust gradients. Fig. 4 shows dust-corrected radial profiles of star formation and the likely growth of bulges in high mass galaxies through in-situ star formation.

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Weitere Publikationen von Autoren mit dem selben Namen

The Radial Distribution of Star Formation in Galaxies at z~1 from the 3D-HST Survey, , , , , , , , , und 9 andere Autor(en). (2013)cite arxiv:1301.0320Comment: Accepted for publication in ApJ Letters.Spatially resolved Halpha maps and sizes of 57 strongly star-forming galaxies at z~1 from 3D-HST: evidence for rapid inside-out assembly of disk galaxies, , , , , , , , , und 6 andere Autor(en). (2012)cite arxiv:1202.1822 Comment: ApJ Letters, in press. The public 3D-HST website is http://3dhst.research.yale.edu/Home.html.The Assembly of Milky Way-like Galaxies Since z~2.5, , , , , , , , , und 9 andere Autor(en). (2013)cite arxiv:1304.2391Comment: Submitted to ApJ Letters. 7 pages, 5 figures.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , und 10 andere Autor(en). (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.Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4, , , , , , , , und . (2015)cite arxiv:1511.04443Comment: Submitted to ApJ Letters. Fig. 2. shows measured radial Balmer decrement profiles. Fig. 3 shows inferred dust gradients. Fig. 4 shows dust-corrected radial profiles of star formation and the likely growth of bulges in high mass galaxies through in-situ star formation.