However, the original Green Bean population show little to
no emission at radio wavelengths.
These so - called relativistic jets produce strong
emission at radio wavelengths.
Not exact matches
Rampadarath explains: «Comparing the VLA images
at radio wavelengths to Chandra's X-ray observations and the hydrogen -
emission detected by Hubble, shows that features are not only connected, but that the
radio outflows are in fact the progenitors of the structures seen by Chandra and Hubble.
Ongoing
radio observations (SMA, JCMT, VLA) of Sirius A are being used to set an observationally determined standard for stellar atmosphere modeling and debris disk studies around A stars, as well as to take the first step toward characterizing potential intrinsic uncertainty in stellar
emission at these
wavelengths.
The
radio emission rose and fell several times, and the relative intensity
at different
radio wavelengths also changed.