¡Nos trasladamos! E-Prints cerrará el 7 de junio.

En las próximas semanas vamos a migrar nuestro repositorio a una nueva plataforma con muchas funcionalidades nuevas. En esta migración las fechas clave del proceso son las siguientes:

Es muy importante que cualquier depósito se realice en E-Prints Complutense antes del 7 de junio. En caso de urgencia para realizar un depósito, se puede comunicar a docta@ucm.es.

The nature of giant clumps in distant galaxies probed by the anatomy of the cosmic snake



Downloads per month over past year

Cava, Antonio and Schaerer, Daniel and Richard, Johan and Pérez González, Pablo Guillermo and Dessauges-Zavadsky, Miroslava and Mayer, Lucio and Tamburello, Valentina (2018) The nature of giant clumps in distant galaxies probed by the anatomy of the cosmic snake. Nature Astronomy, 2 (1). pp. 76-82. ISSN 2397-3366

[thumbnail of perezgonzalez174preprint.pdf]

Official URL: http://dx.doi.org/10.1038/s41550-017-0295-x


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.

Item Type:Article
Additional Information:

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).

Uncontrolled Keywords:Star-forming galaxies; High-redshift galaxies; Lensing cluster; Evolution; Disks; II.; Resolution; Feedback; Regions; Spitzer
Subjects:Sciences > Physics > Astrophysics
Sciences > Physics > Astronomy
ID Code:47068
Deposited On:19 Apr 2018 08:26
Last Modified:10 Dec 2018 15:04

Origin of downloads

Repository Staff Only: item control page