Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

A Long-duration Superflare on the K Giant HD 251108

  • Authors: Hans Moritz Günther, Dheeraj Pasham, Alexander Binks, Stefan Czesla, Teruaki Enoto, Michael Fausnaugh, Franz-Josef Hambsch, Shun Inoue, Hiroyuki Maehara, Yuta Notsu, Jan Robrade, J. H. M. M. Schmitt, P. C. Schneider

Hans Moritz Günther et al 2024 The Astrophysical Journal 977 .

  • Provider: AAS Journals

Caption: Figure 9.

The ﹩0.5\mathrm{log}\sqrt{\mathrm{VEM}}-\mathrm{log}T﹩ diagram for a single-temperature model. The thick, partially transparent blue line is the best fit to the data before MJD = 59901.5 and also describes the data after MJD 59903.3 reasonably well. The thick, partially transparent orange line is the best fit for the period in between. It is much steeper, consistent with little or no reheating. Data shown in this figure are included in the “data behind the figure” for Figure 7.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse