In Pursuit of Supernova Remnants

 
Exploring Extreme Cosmic Phenomena through Multi-Messenger Astronomy and Theoretical Studies

Scientific Information

In Pursuit of Supernova Remnants

 
Supernova remnants (SNRs) play a crucial role in shaping our understanding of the interstellar medium (ISM) and galaxy evolution through shock waves, the enrichment of heavy elements, and cosmic ray production. Recent research highlights the importance of inhomogeneities in the surrounding ISM in driving various high-energy physical processes. For example, dense interstellar clouds that survived shock erosion can produce hadronic gamma-rays through interactions between cosmic-ray protons and interstellar protons. Shock-cloud interactions also enhance turbulent magnetic fields. High-resolution X-ray spectroscopy has begun capturing evidence of thermal X-ray emission resulting from these interactions. Additionally, advances in magnetohydrodynamic simulations have provided new insights into shock interactions with a clumpy gaseous medium, enabling more direct comparisons between numerical simulations and observational data.
 
It is essential to bring together observational and theoretical researchers regularly to exchange and discuss the latest findings related to SNRs. These gatherings not only advance scientific understanding but also play a key role in sustaining and strengthening the research community. Over the past year, groundbreaking observational data from state-of-the-art instruments like XRISM, JWST, and ALMA have emerged, alongside notable progress in theoretical modeling. We hope this workshop will provide a valuable platform for exchanging ideas and further exploration of the nature of SNRs.

SNR Workshop 2025 SOC Chair
Hidetoshi Sano (Gifu University)

Venue

JUROKU PLAZA

 
JUROKU PLAZA adjacent to JR Gifu Station North Exit

Access

  • Website: http://plaza-gifu.jp/index.php
  • Address: 1-10-11 Hashimoto-cho, Gifu City, Gifu 500-8856, Japan
  • Access: A 2-minute walk from JR Gifu Station North Exit.
  • The rapid train from JR Nagoya Station takes approximately 18 minutes to JR Gifu Station. For more details, please refer to the following URL.

Venue

  • Small Conference Room 1 (5th floor, Juroku Plaza)
  • Food and drinks are allowed inside the confarence room.

Lunch

  • You can enjoy meals at the commercial facilities connected to JR Gifu Station (Active G), nearby restaurants, and convenience stores.
  • The restaurant on the 1st floor of JUROKU PLASA is also available.

Accommodation

 

©️ JUROKU PLAZA

 

Small Conference Room 1 (JUROKU PLAZA 5F)

Program

To be determined

Confirmed Invited Speakers

  • Kazumi Kashiyama (Tohoku Univ. | Particle acceleration theory in SNRs)

  • Sei Kato (Paris Institute of Astrophysics / Sorbonne Univ. | Gamma-ray, Neutrino)

  • Toshiki Sato (Meiji Univ. | SNR–SNe relation)

  • Hidetoshi Sano (Gifu Univ.| Shock-cloud interaction)

  • Hiroya Yamaguchi (ISAS/JAXA | XRISM review for SNRs)

  • Danny Milisavljevic (Purdue Univ. | JWST review for SNRs)

Information for Participants

Call for Presentations

  • The deadline for abstract submissions is February 23, 2025.
  • Please submit your title/abstract from this form.
 

General Information

  • Since there will be international participants, we kindly ask that you prepare your talk slides in English.
  • For on-site participants, presentations will be broadcast via Zoom using a MacBook Air at the venue.
  • The presentation language can be either Japanese or English.
  • Your talk slides will be collected before your session. Please check your slides beforehand.
 

Presentation Time※

  • Invited speakers: 40 minutes (30-minute presentation + 10-minute Q&A)
  • Contributed talk: 15 minutes (10-minute presentation + 5-minute Q&A)

※ The presentation time may change depending on the number of participants.

 

Other Information

  • As influenza and other infectious diseases are spreading, we recommend that both on-site participants and speakers wear masks.
  • The venue’s network bandwidth is limited, so we kindly ask on-site participants to avoid connecting to Zoom during the sessions.
  • A reception is planned for the evening of the first day of the workshop. On-site participants will receive a separate email regarding this event, so please register early to participate.

Participants

To be announced

Organizing Committee

Scientific Organizing Committee (SOC)

 

  • Hidetoshi Sano（Gifu Univ., SOC chair）

  • Yasuo Fukui（Nagoya Univ.）

  • Aya Bamba（The Univ. of Tokyo）

  • Takaaki Tanaka（Konan Univ.）

  • Tsuyoshi Inoue（Konan Univ.）

  • Kumiko Nobukawa（Kindai Univ.）

 

Local Organizing Committee (LOC)

 

  • Hidetoshi Sano（Gifu Univ., LOC chair）

  • Takeru Murase（Gifu Univ.）

  • Kisestu Tsuge（Gifu Univ.）

  •  
    • E-mail: sano.hidetoshi.w4[at]f.gifu-u.ac.jp ([at] --> @)

Acknowledgement

This workshop is supported by the JSPS Grant-in-Aid for Scientific Research (A), "Exploring cosmic-ray diffusion processes through a detailed analysis of the ISM [24H00246]" (PI: Hidetoshi Sano).

Last Updated 2025-02-19 / Copyright SNR Workshop 2025. All Rights Reserved.