Resolved gas and dust maps in a z=2 quiescent galaxy reveal accreted material from tidal interactions and a past star-formation rejuvenation, indicating that gas content variations are not solely due to consumption timescales.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
method 1
citation-polarity summary
years
2026 3verdicts
UNVERDICTED 3roles
method 1polarities
use method 1representative citing papers
The -1 km/s absorption toward eta Tel is circumstellar with log C/O < -2.1, matching solar system comet abundances but not carbon-rich disks around hotter stars.
Re-analysis of HST/STIS Lyman-alpha data shows no localized H2O aurora on Europa; a global H exosphere is present with temperature ~1000 K, column density 1.4e12 cm^{-2}, and source rate 1.1e27 s^{-1}.
citing papers explorer
-
Resolved Maps of Gas and Dust in a Massive Quiescent Galaxy at z=2 from INQUEST-JWST: Evidence of Accretion and Rejuvenation
Resolved gas and dust maps in a z=2 quiescent galaxy reveal accreted material from tidal interactions and a past star-formation rejuvenation, indicating that gas content variations are not solely due to consumption timescales.
-
Revisiting the ultraviolet spectroscopy of the eta Tel edge-on debris disk
The -1 km/s absorption toward eta Tel is circumstellar with log C/O < -2.1, matching solar system comet abundances but not carbon-rich disks around hotter stars.
-
Europa's Lyman-$\alpha$ emissions from HST/STIS observations
Re-analysis of HST/STIS Lyman-alpha data shows no localized H2O aurora on Europa; a global H exosphere is present with temperature ~1000 K, column density 1.4e12 cm^{-2}, and source rate 1.1e27 s^{-1}.