Not exact matches
This talk will highlight the effort to characterize
stellar atmospheres through a project known as MESAS (Measuring the Emission of Stellar Atmospheres at Submillimeter / millimeter wavelengths) which is imperative to the success of current and future debris disk s
stellar atmospheres through a project known as MESAS (Measuring the Emission of
Stellar Atmospheres at Submillimeter / millimeter wavelengths) which is imperative to the success of current and future debris disk s
Stellar Atmospheres at Submillimeter / millimeter wavelengths) which is imperative to the success of current and future
debris disk studies.
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.
Researchers looked at 130 single - star systems that the Spitzer Space Telescope had determined to have
debris disks around them and compared them to 277
stellar systems that appeared not to have
debris disks, making this the largest study to observe stars with
debris disks.
We determine that eccentric planets or
stellar companions can induce long - lived eccentric structures in
debris disks.