paper

The quest for stellar coronal mass ejections in late-type stars: I. Investigating Balmer-line asymmetries of single stars in Virtual Observatory data

arXiv:1901.04229 · doi:10.1051/0004-6361/201834264

Abstract

Flares and CMEs can have deleterious effects on their surroundings: they can erode atmospheres of orbiting planets over time and also have high importance in stellar evolution. Most of the CME detections in the literature are single events found serendipitously sparse for statistical investigation. We aimed to gather a large amount of spectral data of M-dwarfs to drastically increase the number of known events to make statistical analysis possible in order to study the properties of potential stellar CMEs. Using archive data we investigated asymmetric features of Balmer-lines, that could indicate the Doppler-signature of ejected material. Of more than 5500 spectra we found 478 with line asymmetries--including nine larger events--on 25 objects, with 1.2-19.6 events/day on objects with line asymmetries. Most events are connected with enhanced Balmer-line peaks, suggesting these are connected to flares similar to solar events. Detected speeds mostly do not reach surface escape velocity: the typical observed maximum velocities are in the order of 100-300km/s , while the typical masses of the ejecta were in the order of g. Statistical analysis suggests that events are more frequent on cooler stars with stronger chromospheric activity. Detected maximum velocities are lower than those observed on the Sun, while event rates were somewhat lower than we could expect from the solar case. These findings may support the idea that most of the CMEs could be suppressed by strong magnetic field. Alternatively, it is possible that we can observe only an early low-coronal phase before CMEs are accelerated at higher altitudes. Our findings could indicate that later-type, active dwarfs could be a safer environment for exoplanetary systems CME-wise than previously thought, and atmosphere loss due to radiation effects would play a stronger role in exoplanetary atmosphere evolution than CMEs.

14 pages, 9 figures, 2 tables, accepted in A&A. Abstract was slightly shortened due to arXiv limits

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