Led by Lavinia Delfini, we use the Gaia XP spectra to derive accretion rates for 145 975 candidate YSO Hα emitters all-sky within 500 pc. We find a percentage of accretors of 70% at 2 Myr and 2.8% at 10 Myr.
Led by Lavinia Delfini, we use the Gaia XP spectra to derive accretion rates for 145 975 candidate YSO Hα emitters all-sky within 500 pc. We find a percentage of accretors of 70% at 2 Myr and 2.8% at 10 Myr.
Great team! And great city! Richard is happy to chat with anyone interested about the role, Leeds, etc.
Great team! And great city! Richard is happy to chat with anyone interested about the role, Leeds, etc.
"Binary interaction via mass transfer causes the Be phenomenon, and triplicity plays a vital role on it"
arxiv.org/abs/2310.05653
"Binary interaction via mass transfer causes the Be phenomenon, and triplicity plays a vital role on it"
arxiv.org/abs/2310.05653
We have studied the clustering properties of forming stars from 1.5 to 20 solar masses as they are traced by the Gaia mission. We find there is an intermediate-mass range (4-10 solar mass) where stars are not that clustered.
Paper:
arxiv.org/abs/2309.00678
We have studied the clustering properties of forming stars from 1.5 to 20 solar masses as they are traced by the Gaia mission. We find there is an intermediate-mass range (4-10 solar mass) where stars are not that clustered.
Paper:
arxiv.org/abs/2309.00678