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Kimura Lab
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A lab exploring high-energy astrophysical phenomena.

AboutAbout the lab
Exploring high-energy astrophysical phenomena and the formation of stars and planets
Kimura Lab studies high-energy astrophysical phenomena, such as gas flows around black holes and the processes occurring in active galactic nuclei.
The lab also investigates electromagnetic waves and neutrinos from objects that emit gravitational waves, the mechanisms by which particles are accelerated, and the origins of cosmic rays and astrophysical neutrinos.
The formation of stars and planets, in particular the dynamics of protoplanetary disks, is also a subject of its research.
Key terms
- Active galactic nucleus
- A region where gas falls onto the black hole at the center of a galaxy and shines extremely brightly
- Cosmic ray
- A particle with very high energy that travels through space
- Neutrino
- A very light elementary particle that barely interacts with matter. Neutrinos also arrive from various astronomical objects in the universe
- Protoplanetary disk
- A disk of gas and dust orbiting a newborn star. It is the place where planets form
ResearchResearch themes
Kimura Lab studies high-energy phenomena that occur in the universe. It also investigates the formation of stars and planets, in particular the dynamics of protoplanetary disks.
View More ↗MembersFaculty
- Associate ProfessorShigeo Kimura
VoicesStudent voices
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Write a lab reviewAnonymous · Your draft is saved if you stopRelatedLabs similar to Kimura Lab
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Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “Anatomy of an Active Galactic Nucleus (SVS14922 - Jet illustrated Loop v01 00001 print)” NASA's Scientific Visualization Studio - NASA’s Goddard Space Flight Center’s Conceptual Image Lab / Public domain (cropped)
- Research on high-energy astrophysical phenomena: “Observatorio de Rayos Gamma HAWC 1” Marifer Veloz / CC BY-SA 4.0 (cropped)
- Related lab (Fujibayashi Lab): “Vela Supernova Remnant - Noirlab2406a” CTIO/NOIRLab/DOE/NSF/AURA Image Processing: T.A. Rector (University of Alaska Anchorage/NSF’s NOIRLab), M. Zamani & D. de Martin (NSF’s NOIRLab) / CC BY 4.0 (cropped)
- Related lab (Kashiyama Lab): “Black hole's accretion disk blank” NASA’s Goddard Space Flight Center/Jeremy Schnittman, cmglee / CC BY-SA 4.0 (cropped)
- Related lab (Toma Lab): “Artist’s illustration of galaxy with jets from a supermassive black hole” ESA/Hubble, L. Calçada (ESO) / CC BY 4.0 (cropped)
- Related lab (Yoshida Lab): “The Star with a Secret Identity” X-ray: NASA/CXC/Huntingdon Inst. for X-ray Astronomy/G.Garmire, Optical: ESO/VLT / Public domain (cropped)
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