Rotational line emission from H2 and HD in dark ages halos is predicted to be nanokelvin for warm halos and a few microkelvins for hot halos, which might be detectable by next-generation telescopes.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.CO 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Hydrogen Molecules in the Dark Ages Halos: Thermal Emission vs. Resonant Scattering
Rotational line emission from H2 and HD in dark ages halos is predicted to be nanokelvin for warm halos and a few microkelvins for hot halos, which might be detectable by next-generation telescopes.