Staratlyon
Du 29/06/2022 au 03/07/2022
Université de Lyon - 92 rue Pasteur, 69007 Lyon
Accueil
COVID-19 INFORMATION:
Dear participants,
We deeply regret to inform you that we have decided to postpone the conference “The Physics of Star Formation: from Stellar Cores to galactic Scales” given the the constantly evolving situation with Covid19 and the impact it has and will keep having on travels in a near future.
We have been closely monitoring the situation in France and around the world over the last weeks. The situation is evolving at different paces in different countries, making travels and large meetings impossible for the next couple of months. We hope that the epidemic expansion will decelerate by June, but the safety and health of all participants is our priority. Besides, we believe that the situation is not in favour of a postponement next fall. We thus have decided to postpone the conference to 2022, around the same period (end of June - early July). 2021 is indeed the year of Protostars and Planets VII where we hope to meet all of you. So please tick already your 2022 agenda at these dates. Meanwhile, we wish the very best to our Japanese colleagues for the PPVII conference !
We deeply thanks the SOC, the invited speakers, and all the participants who applied for a contributed slot (180 in total !). All of you participated in the construction of a promising and high-level program, and we hope to see all of you in Lyon in 2022. The good part of all this involvement is that it should significantly facilitate the organisation of the Star@Lyon 2022.
We will keep you informed in the next couple of months. For those who already registered, please contact us at staratlyon@univ-lyon1.fr to proceed to the reimbursement of the fees.
Les étoiles sont les éléments visibles des structures cosmiques et, à ce titre, elles sont essentielles à notre compréhension de l'Univers et des processus physiques qui régissent leur évolution. La formation des étoiles est un élément moteur du cycle interstellaire qui conduit l'évolution cosmique. Bien que la formation des étoiles soit reconnue comme étant au centre d'un large éventail de processus astrophysiques (formation et évolution des galaxies, évolution et destruction des nuages moléculaires, formation des planètes, et finalement le développement de la vie), elle est l'un des processus les moins bien compris dans l'Univers.Dear participants,
We deeply regret to inform you that we have decided to postpone the conference “The Physics of Star Formation: from Stellar Cores to galactic Scales” given the the constantly evolving situation with Covid19 and the impact it has and will keep having on travels in a near future.
We have been closely monitoring the situation in France and around the world over the last weeks. The situation is evolving at different paces in different countries, making travels and large meetings impossible for the next couple of months. We hope that the epidemic expansion will decelerate by June, but the safety and health of all participants is our priority. Besides, we believe that the situation is not in favour of a postponement next fall. We thus have decided to postpone the conference to 2022, around the same period (end of June - early July). 2021 is indeed the year of Protostars and Planets VII where we hope to meet all of you. So please tick already your 2022 agenda at these dates. Meanwhile, we wish the very best to our Japanese colleagues for the PPVII conference !
We deeply thanks the SOC, the invited speakers, and all the participants who applied for a contributed slot (180 in total !). All of you participated in the construction of a promising and high-level program, and we hope to see all of you in Lyon in 2022. The good part of all this involvement is that it should significantly facilitate the organisation of the Star@Lyon 2022.
We will keep you informed in the next couple of months. For those who already registered, please contact us at staratlyon@univ-lyon1.fr to proceed to the reimbursement of the fees.

Le but de cet atelier est de rassembler les communautés liées à la formation des étoiles à travers les échelles physiques et les temps cosmiques. Ce sujet est particulièrement opportun pour définir les grandes explorations de l'Univers de formation des étoiles qui seront menées dans la prochaine décennie avec de nouveaux instruments conçus pour l'observation et le calcul haute performance exascale. L'état de l'art des trois piliers de l'astrophysique moderne, théorie, observation et simulations numériques, sera représenté. Le programme sera divisé en huit sessions. Chaque session sera couverte par des revues invitées, des présentations invitées ainsi qu'une grande partie réservé pour des contributions orales.
Au plaisir de vous voir à Lyon au début de l'été 2020 !

Topics
1/ Physic and numerics for star formation2/ Isolated star formation: from brown dwarfs to massive stars
3/ Cluster formation
4/ Protostellar disc formation and evolution
5/ Initial Mass Function and Star Formation Rate
6/ Stellar feedback on molecular clouds
7/ Galactic disc formation and evolution
8/ Star formation across redshift
Invited Reviewers
- Nate Bastian (Liverpool John Moores University, UK)- Avishai Dekel (Hebrew University of Jerusalem, Israel)
- James Di Francesco (NRCC, Canada)
- Reinhard Genzel (MPE Garching, Germany)
- Philip Hopkins (CalTech, USA)
- Patrick Hennebelle (CEA Saclay, France)
- Shu-ichiro Inutsuka (University of Nagoya, Japan)
- Diederik Kruijssen (University of Heidelberg, Germany)
- Mark Krumholz (Australian National University, Australia)
- Adam Leroy (Ohio State University, USA)
- Anaëlle Maury (CEA Saclay, France)
- Raffaella Schneider (University of Rome, Italy)
- Kengo Tomida (University of Osaka, Japan)
- Yusuke Tsukamoto (University of Kagoshima, Japan)
- Stefanie Walch (University of Cologne, Germany)