New paper spearheaded by Nadia Blagorodnova and Jakub Klencki on Luminous red nova in NGC 45. For the first time, the progenitor of LRN was analyzed using binary star evolution tracks instead of single star tracks finding that the location exactly matches thermal-timescale (case B) mass transfer in a massive binary. The models suggest that quite a bit of mass (few Msun) was lost from the system in 100s of years before the merger. We take the structure of the final model of the primary and based on standard common envelope formalism predict how much mass should be ejected. We compare this prediction with inference from the transient, modeled as either scaled-down Type II-P or shock-interaction powered. We need transient models calibrated specifically for LRNe! We’re also somewhat puzzled by not seeing a lot of dust in the progenitor – something for future work. https://arxiv.org/abs/2102.05662
We invite applications for a postdoctoral position in the area of computational astrophysics in our research group. The successful candidate will lead development of new computational abilities to understand multi-dimensional evolution of catastrophic interactions of binary stars (mergers, common envelope, compact objects, supernovae). The work will be performed within the project “Cat-In-hAT” funded by the ERC Starting Grant.
Applicants must have a PhD in astronomy, computational physics, or a related field by the start date of the appointment. Candidates with experience with simulations of stellar convection, turbulence, and magnetohydrodynamics are particularly encouraged to apply. The position includes competitive salary and research budget on the level of international fellowships.
We seek 1-2 PhD students to work on topics related to the ERC Starting Grant “Catastrophic interactions of binary stars and the associated transients” (Cat-In-hAT). The work will focus on understanding the theory and observational implications of two merging stars, including neutron stars.
Checkout our website physicsphd.cz/f1. We’ll start accepting applications on December 5 2020 and the deadline is January 15 2021.
Paper led by postdoc Petr Kurfürst explores hydrodynamics of spherical supernova interacting with aspherical CSM. We look at circumstellar disk, bipolar lobes, and shells formed in the wind collision region of binary stars and similar process. While interaction with circumstellar disks (and to some extent with bipolar lobes) leads to expected outcome such as increase in luminosity and double-peaked spectral lines, we find that interaction with colliding wind shells is potentially much more complicated with asymmetric and time-changing line profiles. Cool movies are available on Petr’s website.
Congratulations to Matěj Mezera for successfully defending his Bachelor thesis “Dynamical perturbations of triple stellar and planetary systems seen in gravitational waves with LISA”! In the thesis, he combined three-body integration with gravitational wave strain calculation and Fourier transform.
The book chapter in “Reviews in Frontiers of Modern Astrophysics From Space Debris to Cosmology” has now been published. In addition to basic overview of core-collapse supernova explosion mechanism, the writing includes side-by-side comparisons of predictions of explosion models (explodes yes/no, explosion energy, nickel mass, compact remnant mass) and observational inferences (explosion energy, nickel mass, neutron star mass).
Second (and final) round of computing cluster expansion is finished. Our group now can use a total of 396 cores in 9 normal nodes (each node two 18-core CPUs and 128 GB RAM) and 1 “fat” node (four 18-core CPUs, 512GB RAM). All nodes are connected with 100 Gbps Infiniband and are accessed through a dedicated login node. Big thanks to cluster administrators for trouble-free experience! Picture on the left courtesy of Oldřich Ulrych.
As a part of Prague Doctoral Program we seek 1-2 PhD students to work on topics related to the ERC Starting Grant “Catastrophic interactions of binary stars and the associated transients” (Cat-In-hAT). The work will focus on understanding the theory and observational implications of two merging stars, including neutron stars. Depending on the interests of the student, the work could focus on transients from stellar collisions, (magneto)hydrodynamical evolution of merger products, production of dust and molecules, and understanding the observational counterparts (blue stragglers, R CrB stars, FK Com stars, eta Car, progenitor of SN1987A, GW170817, etc.). The work can utilize existing codes or codes under development in the group: 1D stellar evolution, multidimensional low-Mach number magnetohydrodynamics, moving mesh radiation hydrodynamics, or N-body calculations. In addition, the group is a member of All-Sky Automated Survey for Supernovae, and the thesis can include significant observational or data analysis component.