A Cool Star Flare Reveals an Unexpectedly Hot Emission Component
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| - | [[Image:gj674_cos_lightcurve.png|200px|thumb|right|'''Figure 1''': | + | {{Infobox Nugget |
| + | |name = A Cool Star Flare Reveals an Unexpectedly Hot Emission Component | ||
| + | |title = Nugget Details | ||
| + | |number = 112 | ||
| + | |first_author = C. S. Froning | ||
| + | |second_author = A. Kowalski | ||
| + | |publish_date = September 5, 2019 | ||
| + | |next_nugget = | ||
| + | |previous_nugget = | ||
| + | }} | ||
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| + | ==Introduction== | ||
| + | The [http://cos.colorado.edu/~kevinf/muscles.html MUSCLES and Mega-MUSCLES Treasury Surveys] are large observing programs that are using the Hubble Space Telescope, Chandra X-ray Observatory, XMM-Newton, the Neil Gehrels Swift Observatory, and a suite of ground-based optical telescopes to construct panchromatic (5 Å - 5.5 μm) spectral energy distributions for a representative sample of M dwarf stars (Refs [0],[1]). The goal of the surveys is to establish | ||
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| + | [[Image:gj674_cos_lightcurve.png|200px|thumb|right|'''Figure 1''': During FUV observations with the Hubble Space Telescope, the M2.5V dwarf star, GJ 674, exhibited several small flares and one large flare in the last orbit.]] | ||
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| + | ==Observations and Flare Properties== | ||
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| + | ==Hydrodynamic Models and | ||
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| + | == Conclusion == | ||
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| + | == References == | ||
| + | [0] [https://ui.adsabs.harvard.edu/abs/2016ApJ...820...89F/abstract The MUSCLES Treasury Survey. I. Motivation and Overview] | ||
| + | [1] [https://ui.adsabs.harvard.edu/abs/2017LPICo2042.4052F/abstract Flexing our MUSCLES: The HST Mega-MUSCLES Treasury Survey] | ||
| + | [2] [https://ui.adsabs.harvard.edu/abs/2011Ap%26SS.335..257O/abstract The Cosmic Origins Spectrograph: on-orbit instrument performance] | ||
| + | [3] [https://ui.adsabs.harvard.edu/abs/2019ApJ...871L..26F/abstract A Hot Ultraviolet Flare on the M Dwarf Star GJ 674] | ||
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| + | [[Category: Nugget]] | ||
Revision as of 20:24, 28 August 2019
| A Cool Star Flare Reveals an Unexpectedly Hot Emission Component | |
|---|---|
| Number: | 112 |
| 1st Author: | C. S. Froning |
| 2nd Author: | A. Kowalski |
| Published: | September 5, 2019 |
| Next Nugget: | |
| Previous Nugget: | |
| List all | |
Contents |
Introduction
The MUSCLES and Mega-MUSCLES Treasury Surveys are large observing programs that are using the Hubble Space Telescope, Chandra X-ray Observatory, XMM-Newton, the Neil Gehrels Swift Observatory, and a suite of ground-based optical telescopes to construct panchromatic (5 Å - 5.5 μm) spectral energy distributions for a representative sample of M dwarf stars (Refs [0],[1]). The goal of the surveys is to establish
Observations and Flare Properties
==Hydrodynamic Models and
Conclusion
References
[0] The MUSCLES Treasury Survey. I. Motivation and Overview [1] Flexing our MUSCLES: The HST Mega-MUSCLES Treasury Survey [2] The Cosmic Origins Spectrograph: on-orbit instrument performance [3] A Hot Ultraviolet Flare on the M Dwarf Star GJ 674
Facts about A Cool Star Flare Reveals an Unexpectedly Hot Emission ComponentRDF feed
| RHESSI Nugget Date | 5 September 2019 + |
| RHESSI Nugget First Author | C. S. Froning + |
| RHESSI Nugget Index | 112 + |
| RHESSI Nugget Second Author | A. Kowalski + |
