A search for flares and mass ejections on young late-type stars in the open cluster Blanco-1
arXiv:1406.2734 · doi:10.1093/mnras/stu1161
Abstract
We present a search for stellar activity (flares and mass ejections) in a sample of 28 stars in the young open cluster Blanco-1. We use optical spectra obtained with ESO's VIMOS multi-object spectrograph installed on the VLT. From the total observing time of 5 hours, we find four H flares but no distinct indication of coronal mass ejections (CMEs) on the investigated dK-dM stars. Two flares show "dips" in their light-curves right before their impulsive phases which are similar to previous discoveries in photometric light-curves of active dMe stars. We estimate an upper limit of 4 CMEs per day per star and discuss this result with respect to a semi- empirical estimation of the CME rate of main-sequence stars. We find that we should have detected at least one CME per star with a mass of 1-15 g depending on the star's X-ray luminosity, but the estimated H fluxes associated with these masses are below the detection limit of our observations. We conclude that the parameter which mainly influences the detection of stellar CMEs using the method of Doppler-shifted emission caused by moving plasma is not the spectral resolution or velocity but the flux or mass of the CME.
Accepted for publication in MNRAS, accepted 2014 June 10, received 2014 June 5, in original form 2014 March 24, 14 pages, 5 figures
References in corpus (5)
- Constraining the Age-Activity Relation for Cool Stars: The SDSS DR5 Low-Mass Star Spectroscopic Sample
- The XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue
- Automated Solar Flare Statistics in Soft X-rays over 37 Years of GOES Observations - The Invariance of Self-Organized Criticality during Three Solar Cycles
- The lower mass function of the young open cluster Blanco 1: from 30 Mjup to 3 Mo
- Analysis and modeling of high temporal resolution spectroscopic observations of flares on AD Leo
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