Photospheric and chromospheric activity on EY Dra

✍ Scribed by H. Korhonen; K. Brogaard; K. Holhjem; S. Ramstedt; J. Rantala; C.C. Thöne; K. Vida

• Publisher: John Wiley and Sons
• Year: 2007
• Tongue: English
• Weight: 190 KB
• Volume: 328
• Category: Article
• ISSN: 0004-6337
• DOI: 10.1002/asna.200710777

✦ Synopsis

Abstract

Magnetic activity in the photosphere and chromosphere of the M dwarf EY Dra is studied and possible correlations between the two are investigated using photometric observations in the V and R bands and optical and near infrared spectroscopy. The longitudinal spot configuration in the photosphere is obtained from the V band photometry, and the chromospheric structures are investigated using variations in the H__α__ line profile and observations of the Paschen β line. The shape of the V band light‐curve indicates two active regions on the stellar surface, about 0.4 in phase apart. The spectroscopic observations show enhanced H__α__ emission observed close to the phases of the photometrically detected starspots. This could indicate chromospheric plages associated with the photospheric starspots. Some indications of prominence structures are also seen. The chromospheric pressure is limited to log m~TR~ < –4 based on the non‐detection of emission in the Paschen β wavelength region. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)