Joanna Drążkowska
@astrojoanna.bsky.social
Astrophysicist ✨ Research Group Leader at MPS Göttingen 🇩🇪 Planet formation theory 🪐 she/her
https://www2.mps.mpg.de/homes/drazkowska/
https://www2.mps.mpg.de/homes/drazkowska/
The code can be accessed here github.com/vicky1997/mc...
GitHub - vicky1997/mcdust: 2D Monte Carlo dust evolution code for protoplanetary disks
2D Monte Carlo dust evolution code for protoplanetary disks - vicky1997/mcdust
github.com
July 30, 2025 at 12:55 PM
The code can be accessed here github.com/vicky1997/mc...
See the paper (submitted to @joss-openjournals.bsky.social) here arxiv.org/abs/2507.21239
mcdust: A 2D Monte Carlo code for dust coagulation in protoplanetary disks
mcdust is a parallel simulation code for dust evolution in protoplanetary disks. The code is written in FORTRAN90 and parallelised with OpenMP. The code models dust collisional evolution and transport...
arxiv.org
July 30, 2025 at 12:55 PM
See the paper (submitted to @joss-openjournals.bsky.social) here arxiv.org/abs/2507.21239
I will be there and will be happy to meet you :-)
June 19, 2024 at 9:09 AM
I will be there and will be happy to meet you :-)
Gas disks around young stars are actually not very flat, but dust particles are not pressure-supported (as opposed to the gas) and larger dust aggregates settle to much thinner disks and eventually form flat planetary systems :-)
March 29, 2024 at 4:44 PM
Gas disks around young stars are actually not very flat, but dust particles are not pressure-supported (as opposed to the gas) and larger dust aggregates settle to much thinner disks and eventually form flat planetary systems :-)
I have a couple of colleagues who would qualify but they are not here, LinkedIn is where you find them ;-)
March 29, 2024 at 11:43 AM
I have a couple of colleagues who would qualify but they are not here, LinkedIn is where you find them ;-)