Synapse
⌘+K
Synapse
PulseExploreClubsResearchersJournals
Instagram
HomeClubsExplore
April 17, 2014Monthly Notices of the Royal Astronomical SocietyOpen Access

A signature of chromospheric activity in brown dwarfs revealed by 2.5–5.0 μm AKARI spectra

View Full Paper
Ask AI
Bookmark
Share

Authors

SSSatoko SorahanaNagoya UniversityTST. K. SuzukiIYI. YamamuraJapan Aerospace Exploration Agency

Discussion

Loading...

Member takes

Implication

Key Points

Key points are not available for this paper at this time.

Cite This Study

Sorahana et al. (2014) studied this question.

synapsesocial.com/papers/6a94d758efe1bb9e53eff201https://doi.org/10.1093/mnras/stu479
View Full Paper
Ask AI
Bookmark
Share

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

  1. 1A new model for brown dwarf spectra including accurate unified line shape theory for the Na I and K I resonance line profiles2003 · 140 citations
  2. 2Confirmation of the Electron Cyclotron Maser Instability as the Dominant Source of Radio Emission from Very Low Mass Stars and Brown Dwarfs2008 · 245 citations
  3. 3Dust in the Photospheric Environment: Unified Cloudy Models of M, L, and T Dwarfs2002 · 167 citations
  4. 4The theory of brown dwarfs and extrasolar giant planets2001 · 823 citations
  5. 5Chromospheric Activity, Rotation, and Rotational Braking in M and L Dwarfs2008 · 262 citations