Synapse
⌘+K
Synapse
PulseExploreClubsResearchersJournals
Instagram
HomeClubsExplore
August 26, 2008The Astrophysical JournalOpen Access

Confirmation of the Electron Cyclotron Maser Instability as the Dominant Source of Radio Emission from Very Low Mass Stars and Brown Dwarfs

View Full Paper
Ask AI
Bookmark
Share

Authors

GHGregg HallinanCalifornia Institute of TechnologyAAA. AntonovaInstitute of Astronomy and National Astronomical ObservatoryJDJ. G. DoyleArmagh Observatory & Planetarium

Discussion

Loading...

Member takes

Implication

Key Points

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

Cite This Study

Hallinan et al. (2008) studied this question.

synapsesocial.com/papers/69d78790f07a12db70b8b283https://doi.org/10.1086/590360
View Full Paper
Ask AI
Bookmark
Share

Also Consider

Synapse has enriched 4 closely related papers on similar clinical questions. Consider them for comparative context:

  1. 1Quiescent Radio Emission from Southern Late‐Type M Dwarfs and a Spectacular Radio Flare from the M8 Dwarf DENIS 1048−39562005 · 100 citations
  2. 2Activity and Kinematics of Ultracool Dwarfs, Including an Amazing Flare Observation2007 · 200 citations
  3. 3Rotational Modulation of the Radio Emission from the M9 Dwarf TVLM 513−46546: Broadband Coherent Emission at the Substellar Boundary?2006 · 157 citations
  4. 4GU Bootis: A New 0.6<i>M</i><sub>⊙</sub>Detached Eclipsing Binary2005 · 183 citations