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Study mode:
on
1
Introduction
2
Science Motivation
3
Common Envelope
4
Discs
5
Background
6
Post HP binaries
7
Gas vs dust
8
Binary evolution
9
Do we need it
10
What do we need
11
What is SS433
12
Mass loss
13
How many will merge
14
Stellar mergers
15
How jets and winds affect orbital evolution
16
Mass ratio
17
Specific momentum
18
Isotropic
19
Simulation Results
20
Zoom Questions
21
Parameter Space Exploration
22
Questions
23
Distractions
24
Behavior
25
Inflow
26
Conclusion
Description:
Explore orbital evolution in binary systems through this conference talk from the Building Bridges conference at KITP. Delve into the complexities of circumbinary gas, its evolution, and influence on embedded binaries. Examine observational signatures, numerical modeling techniques, and the similarities between massive black hole binaries and stellar binaries. Gain insights from experts Selma De Mink and Sophie Schroder as they discuss topics such as common envelopes, discs, post-HP binaries, gas vs. dust dynamics, and the importance of binary evolution in understanding these systems. Learn about mass loss, merger rates, stellar mergers, and the effects of jets and winds on orbital evolution. Discover simulation results, parameter space exploration, and key questions in the field of binary system evolution.

Orbital Evolution I - Selma De Mink, Sophie Schroder

Kavli Institute for Theoretical Physics
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