I am looking for Bachelor & Master students. Here is a (non-exhaustive) list of possible topics:
Dynamical perturbations of triple stellar and planetary systems seen in gravitational waves with LISA
Looking over the cliff: when do close binary stars merge?
Combining astrometry a variability information from the Gaia satellite
Radiation transport on exploding background and applications to supernovae, stellar mergers, and classical novae
Stellar merger model for the progenitor of SN1987A
All topics are related to research of current interest supported by grants and should result in one or more scientific papers. The thesis topic is always finalized upon discussions with the student. The methods of work include semi-analytic calculations, (radiation) hydrodynamics, and statistical analysis of data.
I’m one of the co-organizers of RAS Specialist Discussion meeting on common envelopes, mergers, and related fun to be held in London on October 11 2019. Abstracts are due by the end of this August. The meeting website is https://commonenvelopes.space/
In a paper led by David Jones with Romano Corradi from La Palma we tried to come up with a theory to explain the peculiar shape (including new distant emission regions firstly presented here) and central stars of the planetary nebula. Our preferred models includes Lidov-Kozai cycles and triple star disruption due to ejection of the planetary nebula.
Thanks to our ERC grant, we have commenced upgrading the computing cluster Sněhurka (Snow White). In the first step, we got a new Infiniband switch and 5 new nodes with 36 cores each. Looking forward to new results!
Dominika Hubova expanded her Bachelor thesis and took the deepest look so far at ballistic mass loss from L2, focusing on what happens if the matter stream is initiated with offset from L2 and with a velocity kick. Dominika characterized the parameter space and found some new stream trajectories. Interestingly, even if the stream is launched slower than corotation, there are still many initial positions near L2 that provide sufficient tidal torque to unbind the material.
A paper characterizing periodic and aperiodic variability of APOGEE targets with ASAS-SN data was recently accepted to MNRAS. In this effort led by Michał Pawlak, we characterized almost 2000 periodic variable stars, all with existing multi-epoch high-resolution spectroscopy from APOGEE. We found that eclipsing binaries tend to favor lower metallicities, as was recently found on purely spectroscopic samples. We characterized the variability with damped random walk stochastic process. This is a starting point for future investigations combining high-res spectroscopy from surveys with time-domain photometric information. The paper is available on astro-ph.