
Explore observational tests of binary system theories, focusing on circumbinary gas evolution and its influence on embedded binaries across stellar and black hole scales.

Explore observational tests of binary systems in astrophysics, from stellar pairs to supermassive black holes, and their interactions with surrounding gas in this insightful conference talk.

Explore circumbinary gas evolution, observational signatures, and numerical modeling techniques in stellar and black hole binary systems with experts Roger Blandford and Sean McWilliams.

Explore binary systems in astrophysics, from stellar to supermassive black holes. Discuss gas evolution, observational signatures, and numerical modeling techniques across varied scales.

Explore the evolution and influence of circumbinary gas in binary systems, from stellar to supermassive black holes, and its observational signatures across astrophysical scales.

Explore electromagnetic observations of binary supermassive black holes and new opportunities with large synoptic surveys. Gain insights into circumbinary gas evolution and its influence on embedded binary systems.

Explore circumbinary gas evolution, observational signatures, and numerical modeling techniques for binary systems across stellar and black hole scales.

Explore dual AGN properties from kiloparsec scales to merger, focusing on systems that become gravitational wave sources. Gain insights into circumbinary gas evolution and its influence on binary systems.

Explore the evolution of supermassive black hole binaries from galaxy mergers to gravitational waves, examining their interactions with circumbinary gas and observational signatures.

Explore circumbinary gas evolution in stellar and black hole binary systems, examining observational signatures and numerical modeling techniques to advance our understanding of these complex astrophysical phenomena.

Explore the impact of accretion on gravitational wave source formation in binary systems, from stellar to supermassive black hole scales, with insights on circumbinary gas evolution and observational signatures.

Explore extreme white dwarfs: their unique properties, recent discoveries, and implications for stellar evolution. Learn about cutting-edge research using advanced telescopes and instruments to uncover mysteries of these dense stellar remnants.

Explore spectral prediction and assignment techniques for strongly magnetized systems, focusing on white dwarf stars and their astrophysical implications in galactic population studies.

Explore surviving stellar remnants from thermonuclear supernovae with Roberto Raddi. Discover astrometric, photometric, and spectroscopic insights into white dwarfs and their role in understanding galactic evolution.

Explore observations of polluted white dwarfs, their significance in astrophysics, and insights into stellar and planetary evolution. Gain expert knowledge on this fascinating topic in astronomy.

Explore white dwarf pollution through astrometric, photometric, and spectroscopic data. Gain insights into stellar remnants and their role in probing various astrophysical phenomena.

Exploring the journey from supernova remnants to white dwarfs, this talk delves into stellar evolution, offering insights into Galactic populations and astrophysical phenomena.

Explore how infant-phase signals from supernova SN2018aoz provide insights into white dwarf physics and stellar evolution, presented by Yuan Qi Ni from the University of Toronto.

Explore thermonuclear supernovae observations with Kate Maguire, covering astrometric, photometric, and spectroscopic data from all-sky surveys to gain insights into white dwarf populations and their astrophysical implications.

Explore multidimensional hydrodynamical simulations and radiative transfer in white dwarf astrophysics. Gain insights into advanced modeling techniques for studying stellar remnants and their implications for galactic evolution.

Explore Type Ia supernova progenitors with Ruediger Pakmor, focusing on white dwarf physics, stellar evolution, and their role in galactic populations and gravitational wave sources.