CORONAL MASS EJECTIONS AS A MECHANISM FOR PRODUCING IR VARIABILITY IN DEBRIS DISKS
- 26 February 2013
- journal article
- Published by American Astronomical Society in The Astrophysical Journal Letters
- Vol. 765 (2) , L44
Abstract
No abstract availableAll Related Versions
This publication has 14 references indexed in Scilit:
- GLOBAL ENERGETICS OF THIRTY-EIGHT LARGE SOLAR ERUPTIVE EVENTSThe Astrophysical Journal, 2012
- Rapid disappearance of a warm, dusty circumstellar diskNature, 2012
- Search for indications of stellar mass ejections using FUV spectraAstronomy & Astrophysics, 2011
- Solar Flares and Coronal Mass Ejections: A Statistically Determined Flare Flux – CME Mass CorrelationSolar Physics, 2010
- The SOHO/LASCO CME CatalogEarth, Moon, and Planets, 2009
- Properties of Interplanetary Coronal Mass EjectionsSpace Science Reviews, 2007
- On the CME velocity distributionAstronomy & Astrophysics, 2006
- Refinements to flare energy estimates: A followup to “Energy partition in two solar flare/CME events” by A. G. Emslie et al.Journal of Geophysical Research, 2005
- ChandraObservations of the Pleiades Open Cluster: X‐Ray Emission from Late B‐ to Early F‐Type BinariesThe Astrophysical Journal, 2002
- A Possible Massive Asteroid Belt around ζ LeporisThe Astrophysical Journal, 2001