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Fo Guang Shan

Taiwan

1 paper here3 citations across 1
fields
  • astro-ph.GA1
ROR 04a092p69OpenAlex

affiliations via OpenAlex

most citedThe factors that influence protostellar multiplicity I: Gas temperature, density, and mass in Perseus with Nobeyama

3 citations

researchers with a paper here
  • A. Hacar1
  • Christina Fuchs1
  • D. Harsono1
  • Doug Johnstone1
  • J. J. Tobin1
  • M. V. Persson1
  • Nami Sakai1
  • N. M. Murillo1
  • R. Mignon-Risse1
  • Shaoshan Zeng1
  • Timothy H. Hsieh1
  • Y. Yang1
collaborating institutions
  • Centre National de la Recherche ScientifiqueFR1 paper
  • Hallands sjukhus KungsbackaSE1 paper
  • Herzberg Institute of AstrophysicsCA1 paper
  • Laboratoire AstroParticule et CosmologieFR1 paper
  • Max Planck Institute for Extraterrestrial PhysicsDE1 paper
  • National Radio Astronomy ObservatoryUS1 paper
  • National Tsing Hua UniversityTW1 paper
  • Norwegian University of Science and TechnologyNO1 paper
  • Pioneer (United States)US1 paper
  • RIKENJP1 paper
  • Universidad Nacional Autónoma de MéxicoMX1 paper
  • Université Paris CitéFR1 paper

1 paper

astro-ph.GA2024★ 3 cited

The factors that influence protostellar multiplicity I: Gas temperature, density, and mass in Perseus with Nobeyama

N. M. Murillo, C. M. Fuchs, D. Harsono +9

Protostellar multiplicity is common at all stages and mass ranges. However, the factors that determine the multiplicity of protostellar systems have not been systematically charact…

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