RT Journal Article
T1 The nature of giant clumps in distant galaxies probed by the anatomy of the cosmic snake
A1 Cava, Antonio
A1 Schaerer, Daniel
A1 Richard, Johan
A1 Pérez González, Pablo Guillermo
A1 Dessauges-Zavadsky, Miroslava
A1 Mayer, Lucio
A1 Tamburello, Valentina
AB Giant stellar clumps are ubiquitous in high-redshift galaxies(1,2). They are thought to play an important role in the build-up of galactic bulges(3) and as diagnostics of star formation feedback in galactic discs(4). Hubble Space Telescope (HST) blank field imaging surveys have estimated that these clumps have masses of up to 10(9.5) M-circle dot and linear sizes of greater than or similar to 1 kpc(5,6). Recently, gravitational lensing has also been used to get higher spatial resolution(7-9). However, both recent lensed observations(10,11) and models(12,13) suggest that the clumps' properties may be overestimated by the limited resolution of standard imaging techniques. A definitive proof of this observational bias is nevertheless still missing. Here we investigate directly the effect of resolution on clump properties by analysing multiple gravitationally lensed images of the same galaxy at different spatial resolutions, down to 30 pc. We show that the typical mass and size of giant clumps, generally observed at similar to 1 kpc resolution in high-redshift galaxies, are systematically overestimated. The high spatial resolution data, only enabled by strong gravitational lensing using currently available facilities, support smaller scales of clump formation by fragmentation of the galactic gas disk via gravitational instabilities.
PB Nature Publishing Group
SN 2397-3366
YR 2018
FD 2018-01
LK https://hdl.handle.net/20.500.14352/12024
UL https://hdl.handle.net/20.500.14352/12024
LA eng
NO The work of A.C., D.S., M.D.-Z.,L.M. and V.T. is supported by the STARFORM Sinergia Project funded by the Swiss National Science Foundation. J.R. acknowledges support from the European Research Council starting grant 336736-CALENDS. P.G. P.-P. acknowledges support from Spanish Government MINECO grants AYA2015-70815-ERC and AYA2015-63650-P. This work has made use of the Rainbow Cosmological Surveys Database, which is operated by the Universidad Complutense de Madrid (UCM), partnered with the University of California Observatories at Santa Cruz (UCO/Lick, UCSC). Based on observations made with the NASA/ESA Hubble Space Telescope, and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST- ECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA).
NO Unión Europea. FP7
NO Ministerio de Economía y Competitividad (MINECO)
NO STARFORM Sinergia Project - Swiss National Science Foundation
DS Docta Complutense
RD 8 may 2024