Energetic flares on RS CVn stars
نویسندگان
چکیده
منابع مشابه
Musicos 1998: Optical and X-rays Observations of Flares on the Rs Cvn Binary Hr 1099
We present simultaneous and continuous observations of Hα, Hβ, Na i D1, D2 and He i D3 lines of the chromospherically active binary HR 1099. We have observed HR 1099 for more than 3 weeks almost continuously and monitored two flares. An increase in Hα, Ca ii H & K, Hβ, Hei D3 and Hei λ6678 and a strong filling-in of the Nai D1, D2 and Mgi b triplet during one of the flares are observed. We have...
متن کاملMusicos 1998: Observations of Rotational Modulation and Flares on the Rs Cvn Binary Hr1099
We present simultaneous and continuous observations of Hα, Hβ, Na I D 1 , D 2 , He I D 3 and Ca II H & K lines of the chromospherically active binary HR 1099. We have observed HR 1099 for more than 3 weeks almost continuously and monitored two flares. An increase in Hα and Ca II H & K, Hβ and He I D 3 and a strong filling-in of the Na I D 1 , D 2 during the flares are observed. We have found th...
متن کاملSimultaneous Optical and X-ray Observations of Flares and Rotational Modulation on the RS CVn
We present simultaneous and continuous observations of the Hα, Hβ, He i D3, Na i D1,D2 doublet and the Ca ii H & K lines for the RS CVn system HR 1099. The spectroscopic observations were obtained during the MUSICOS 1998 campaign involving several observatories and instruments, both echelle and long-slit spectrographs. During this campaign, HR 1099 was observed almost continuously for more than...
متن کاملLetter to the Editor Permanent active longitudes and activity cycles on RS CVn stars
A new analysis of the published long-term photometric observations has revealed permanent active-longitude structures in four RS CVn stars: EI Eri, II Peg, σ Gem, and HR 7275. Two active longitudes separated by half of the period are found to dominate on the surface during all available seasons. The positions of the longitudes on three stars (EI Eri, II Peg, HR 7275) are migrating in the orbita...
متن کاملAM CVn stars
I review our observational and theoretical knowledge of AM CVn stars, focusing on recent developments. These include newly discovered systems, the possibility that two recently discovered extremely short period objects are AM CVn stars and an update on X-ray, UV an optical studies. Theoretical advances include the study of the details of both the donor and accretor, and the physics of the heliu...
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ژورنال
عنوان ژورنال: International Astronomical Union Colloquium
سال: 1989
ISSN: 0252-9211
DOI: 10.1017/s0252921100153941