Type II supernovae happen in single star systems (or at least far enough away from any companion star to retain their hydrogen outer layers) and have
strong hydrogen emission lines.
Type I supernovae happen in close binary systems and do not show
strong hydrogen emission lines.
Not exact matches
Type Ib and Ic supernovae result from the collapse of a massive star's core whose outer
hydrogen layers have been transfered to a companion star or blown off from
strong winds which is why they do not show
hydrogen emission lines.
Hydrogen emission from EGSY8p7 may indicate it is the first known example of an early generation of young galaxies emitting unusually
strong radiation.
Using Keck Observatory's powerful infrared spectrograph called MOSFIRE, the team dated the galaxy by detecting its Lyman - alpha
emission line — a signature of hot
hydrogen gas heated by
strong ultraviolet
emission from newly born stars.
A new National Research Council report finds that by the year 2050, the U.S. may be able to reduce petroleum consumption and greenhouse gas
emissions by 80 percent for light - duty vehicles — cars and small trucks — via a combination of more efficient vehicles; the use of alternative fuels like biofuels, electricity, and
hydrogen; and
strong government policies to overcome high costs and influence consumer choices.