Search Publications

Strong damped Lyman-α absorption in young star-forming galaxies at redshifts 9 to 11
DOI: 10.1126/science.adj0343 Bibcode: 2024Sci...384..890H

Finkelstein, Steven L.; Arrabal Haro, Pablo; Heintz, Kasper E. +18 more

Primordial neutral atomic gas, mostly composed of hydrogen, is the raw material for star formation in galaxies. However, there are few direct constraints on the amount of neutral atomic hydrogen (H I) in galaxies at early cosmic times. We analyzed James Webb Space Telescope (JWST) near-infrared spectroscopy of distant galaxies, at redshifts ≳8. Fr…

2024 Science
Gaia JWST 91
A far-ultraviolet–driven photoevaporation flow observed in a protoplanetary disk
DOI: 10.1126/science.adh2861 Bibcode: 2024Sci...383..988B

Hartigan, Patrick; Zhang, Yong; Gordon, Karl D. +144 more

Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiation produces photodissociation regions (PDRs) on the surfaces of protoplanetary disks around low-mass stars, which affects planet formation within the disks. We report Ja…

2024 Science
eHST JWST 25
Abundant hydrocarbons in the disk around a very-low-mass star
DOI: 10.1126/science.adi8147 Bibcode: 2024Sci...384.1086A

Waters, L. B. F. M.; Olofsson, G.; Kamp, I. +40 more

Very-low-mass stars (those less than 0.3 solar masses) host orbiting terrestrial planets more frequently than other types of stars. The compositions of those planets are largely unknown but are expected to relate to the protoplanetary disk in which they form. We used James Webb Space Telescope mid-infrared spectroscopy to investigate the chemical …

2024 Science
XMM-Newton JWST 22
Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A
DOI: 10.1126/science.adj5796 Bibcode: 2024Sci...383..898F

Fox, O. D.; Blommaert, J. A. D. L.; Larsson, J. +31 more

The nearby Supernova 1987A was accompanied by a burst of neutrino emission, which indicates that a compact object (a neutron star or black hole) was formed in the explosion. There has been no direct observation of this compact object. In this work, we observe the supernova remnant with JWST spectroscopy, finding narrow infrared emission lines of a…

2024 Science
Gaia JWST 22
A magnified compact galaxy at redshift 9.51 with strong nebular emission lines
DOI: 10.1126/science.adf5307 Bibcode: 2023Sci...380..416W

Koekemoer, Anton M.; Treu, Tommaso; Broadhurst, Tom +21 more

Ultraviolet light from early galaxies is thought to have ionized gas in the intergalactic medium. However, there are few observational constraints on this epoch because of the faintness of those galaxies and the redshift of their optical light into the infrared. We report the observation, in JWST imaging, of a distant galaxy that is magnified by g…

2023 Science
Gaia eHST JWST 103
The distribution of CO2 on Europa indicates an internal source of carbon
DOI: 10.1126/science.adg4155 Bibcode: 2023Sci...381.1308T

Brown, Michael E.; Trumbo, Samantha K.

Jupiter’s moon Europa has a subsurface ocean, the chemistry of which is largely unknown. Carbon dioxide (CO2) has previously been detected on the surface of Europa, but it was not possible to determine whether it originated from subsurface ocean chemistry, was delivered by impacts, or was produced on the surface by radiation processing …

2023 Science
JWST 33