We characterize
the main emission lines found in the spectrum, which primarily arise from a range of components associated with Orion KL including the hot core, but also see widespread emission from components associated with molecular outflows traced by H2O, SO2, and OH.
We characterize
the main emission lines found in the spectrum, which primarily arise from a range of components associated with Orion KL including the hot core, but... ▽ More We present the first high spectral resolution observations of Orion KL in the frequency ranges 1573.4 - 1702.8 GHz (band 6b) and 1788.4 - 1906.8 GHz (band 7b) obtained using the HIFI instrument on board the Herschel Space Observatory.
Not exact matches
Massive yet non-supergiant entities known as «Be stars» are
main - sequence stars that notably have, or had at some time, one or more Balmer
lines in
emission, with the hydrogen - related electromagnetic radiation series projected out by the stars being of particular interest.
The bottom
line is, if you're in a village — even in a highlands region facing more mosquitoes — is your
main concern a global blunting of
emissions of greenhouse gases or access to insecticides and mosquito nets?
So, it's hard to see how the yellow
line (carbon dioxide
emissions) could be the
main reason for changes in the red
line.
Designed well, both of these approaches can deliver on the
main aim of a robust carbon pricing program, which is to help cut
emissions cost - effectively in
line with climate and energy goals.