Yanqihu Campus,
the University of Chinese Academy of Sciences,
380 Huaibeizhuang, Huairou District,
Beijing, China
Lectures will take place simultaneously in two cohorts, A and B. On the first day, please find out which cohort you belong to.
MONDAY 6/25 Introduction |
TUESDAY 6/26 Globular Clusters |
WEDNESDAY 6/27 Massive Stars |
THURSDAY 6/28 Binaries |
FRIDAY 6/29 WD novae |
|
---|---|---|---|---|---|
8:30 AM | Lecture Getting started with MESA |
Lecture Globular Clusters |
Lecture Massive Stellar Evolution |
Lecture Current developments in binary evolution |
Lecture Introduction to novae |
9:20 AM | Minilab Inlists and 1M to WD |
Minilab Exploring Cluster Data |
Minilab Crowdsource parameter study on resolution |
Minilab Modeling high mass BH X-ray binaries |
Lab A first nova model |
10:10 AM | Break | Break | Break | Break | Break |
10:30 AM | Maxilab PG-Plot |
Lecture Stellar Atmospheres |
Lecture Run massive stellar evolution |
MaxiLab Orbital evolution of binary systems |
Lecture Nuclear physics of novae |
11:20 AM | Maxilab PG-Plot |
Minilab Translating MESA results to observable |
Minilab from Oxygen Core to Fe core collapse |
Maxilab The Algol paradox |
Lab Exploring nuclear networks in MESA |
12:10 AM | Lunch | Lunch | Lunch | Lunch | Lunch |
1:30 PM | Lecture Stellar Evolution: All about MESA |
Lecture White Dwarfs |
Lecture Mixing in Massive Stars and Pre-supernova Structure |
Lecture Common envelope evolution |
Lecture Mass loss in novae |
2:20 PM | Minilab High mass stars |
Minilab White-Dwarf Luminosity Functions |
Minilab Visualize the effects of different mixing with PG-Plot |
Minilab The binding energy of stellar envelopes |
Lab The role of mass loss in nova models |
3:10 PM | Break | Break | Break | Break | Break |
3:30 PM | Lecture Customizing with run_star_extra |
Lecture Testing Physics with White Dwarfs |
Lecture Magnetorotational instability and massive stars |
Lecture Formation of BH X-ray binaries |
Lecture Open issues in the physics of novae |
4:20 PM | Maxilab run_star_extra |
Maxilab Neutrinos, Axions, Gravity |
Maxilab Import an analytic description of MRI into MESA |
Maxilab BH X-ray binaries from common envelope evolution |
Lab Mixing and enrichment in novae |
5:10 PM | Dinner | Dinner | Dinner | Dinner | Dinner |
7:00 PM | Catch up session | Catch up session | Catch up session | Catch up session | Catch up session |
MONDAY 6/25 Introduction |
TUESDAY 6/26 Massive Stars |
WEDNESDAY 6/27 Globular Clusters |
THURSDAY 6/28 WD Novae |
FRIDAY 6/29 Binaries |
|
---|---|---|---|---|---|
8:30 AM | Lecture Getting started with MESA |
Lecture Massive Stellar Evolution |
Lecture Globular Clusters |
Lecture Introduction to novae |
Lecture Current developments in binary evolution |
9:20 AM | Minilab Inlists and 1M to WD |
Minilab Crowdsource parameter study on resolution |
Minilab Exploring Cluster Data |
Lab A first nova model |
Minilab Modeling high mass BH X-ray binaries |
10:10 AM | Break | Break | Break | Break | Break |
10:30 AM | Maxilab PG-Plot |
Lecture Run massive stellar evolution |
Lecture Stellar Atmospheres |
Lecture Nuclear physics of novae |
MaxiLab Orbital evolution of binary systems |
11:20 AM | Maxilab PG-Plot |
Minilab from Oxygen Core to Fe core collapse |
Minilab Translating MESA results to observable |
Lab Exploring nuclear networks in MESA |
Maxilab The Algol paradox |
12:10 AM | Lunch | Lunch | Lunch | Lunch | Lunch |
1:30 PM | Lecture Stellar Evolution: All about MESA |
Lecture Mixing in Massive Stars and Pre-supernova Structure |
Lecture White Dwarfs |
Lecture Mass loss in novae |
Lecture Common envelope evolution |
2:20 PM | Minilab High mass stars |
Minilab Visualize the effects of different mixing with PG-Plot |
Minilab White-Dwarf Luminosity Functions |
Lab The role of mass loss in nova models |
Minilab The binding energy of stellar envelopes |
3:10 PM | Break | Break | Break | Break | Break |
3:30 PM | Lecture Customizing with run_star_extra |
Lecture Magnetorotational instability and massive stars |
Lecture Testing Physics with White Dwarfs |
Lecture Open issues in the physics of novae |
Lecture Formation of BH X-ray binaries |
4:20 PM | Maxilab run_star_extra |
Maxilab Import an analytic description of MRI into MESA |
Maxilab Neutrinos, Axions, Gravity |
Maxilab Mixing and enrichment in novae |
Maxilab BH X-ray binaries from common envelope evolution |
5:10 PM | Dinner | Dinner | Dinner | Dinner | Dinner |
7:00 PM | Catch up session | Catch up session | Catch up session | Catch up session | Catch up session |
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Yanqihu Campus,
the University of Chinese Academy of Sciences,
380 Huaibeizhuang, Huairou District,
Beijing, China
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Yanqihu Campus,
the University of Chinese Academy of Sciences,
380 Huaibeizhuang, Huairou District,
Beijing, China