- Title
- The factors that influence protostellar multiplicity: I. Gas temperature, density, and mass in Perseus with Nobeyama
- Creators
- N. M. Murillo - RIKENC. M. Fuchs - Fox2Space - FTSCO, The Fault Tolerant Satellite Computer Organization, Linz, AustriaD. Harsono - National Tsing Hua UniversityN. Sakai - RIKENA. Hacar - University of ViennaD. Johnstone - Herzberg Institute of AstrophysicsR. Mignon-Risse - Université Paris CitéS. Zeng - RIKENT. H. Hsieh - Max Planck Institute for Extraterrestrial PhysicsY. L. Yang - RIKENJ. J. Tobin - National Radio Astronomy ObservatoryM. V. Persson - Kungsbacka, Sweden
- Grant note
- NRC Canada Ministry of Education, Culture, Sports, Science and Technology (http://data.elsevier.com/vocabulary/SciValFunders/501100001700) 111B3005191 / National Science and Technology Council (http://data.elsevier.com/vocabulary/SciValFunders/100020595) Centre National d’Etudes Spatiales (http://data.elsevier.com/vocabulary/SciValFunders/501100002830) 20H05844; 20H05645; 20H05845 / Ministry of Education, Culture, Sports, Science and Technology (http://data.elsevier.com/vocabulary/SciValFunders/501100001700) National Science and Technology Council (http://data.elsevier.com/vocabulary/SciValFunders/100020595) Horizon 2020 (http://data.elsevier.com/vocabulary/SciValFunders/501100007601) Ministry of Education (http://data.elsevier.com/vocabulary/SciValFunders/100010002) RIKEN (http://data.elsevier.com/vocabulary/SciValFunders/501100006264) r-EMU
- Resource Type
- Journal article
- Date published
- 01/09/2024
- Publication Details
- Astronomy and astrophysics (Berlin), Vol.689, p.A267
- Language
- English
Journal article
The factors that influence protostellar multiplicity: I. Gas temperature, density, and mass in Perseus with Nobeyama
Astronomy and astrophysics (Berlin), Vol.689, p.A267
01/09/2024
Metrics
1 Record Views