JWST mid-IR spectroscopy shows LHS 3844 b has a dark, space-weathered, low-silica surface with no evidence of accumulated CO2 or SO2 gases.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
dataset 1
citation-polarity summary
years
2026 2roles
dataset 1polarities
use dataset 1representative citing papers
A bow shock around a diskless polar cataclysmic variable requires persistent power exceeding accretion energy, pointing to a new magnetic energy-loss mechanism that may affect binary evolution.
citing papers explorer
-
The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy
JWST mid-IR spectroscopy shows LHS 3844 b has a dark, space-weathered, low-silica surface with no evidence of accumulated CO2 or SO2 gases.
-
A persistent bow shock in a diskless magnetised accreting white dwarf
A bow shock around a diskless polar cataclysmic variable requires persistent power exceeding accretion energy, pointing to a new magnetic energy-loss mechanism that may affect binary evolution.