posted on 2017-07-31, 13:03authored byK. R. Briggs, J. P. Pye
We present the first results from a 40 ks Guaranteed Time XMM-Newton pointing in the Pleiades. We detect almost all early-mid dM members in the field and several very low mass (VLM) stars - including the brown dwarf (BD) candidate Roque 9 - and investigate the variation of X-ray activity levels, hardness ratios and flare frequency with spectral type down to the BD regime.
History
Citation
ASP Conference: Stellar coronae in the Chandra and XMM-Newton Era, pp. 437-442
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
AM (Accepted Manuscript)
Published in
ASP Conference: Stellar coronae in the Chandra and XMM-Newton Era