activity
20002023
most citedSolar-type dynamo behaviour in fully convective stars without a tachocline

207 citations · 2.6k across the 99 of their papers we have counts for

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Showing 2006 · astro-phShow all

5 papers · 2 filters

astro-ph2006★ 19 cited

TeV J2032+4130: a not-so-dark Accelerator?

Yousaf M. Butt, Jorge A. Combi, Jeremy Drake +5

The HEGRA gamma-ray source TeV J2032+4130 is considered the prototypical 'dark accelerator', since it was the first TeV source detected with no firm counterparts at lower frequenci…

astro-ph2006

Soft X-ray Spectroscopy of the Hot DA White Dwarf LB1919 and the PG1159 Star PG1520+525

K. Werner, J. J. Drake, T. Rauch +2

We have performed soft X-ray spectroscopy of two hot white dwarfs with the Chandra observatory using the Low Energy Transmission Grating. The first target is the hot DA white dwarf…

astro-ph2006★ 21 cited

Infrared observations of the 2006 outburst of the recurrent nova RS Ophiuchi: the early phase

A. Evans, T. Kerr, Bin Yang +20

We present infrared spectroscopy of the recurrent nova RS Ophiuchi, obtained 11.81, 20.75 and 55.71 days following its 2006 eruption. The spectra are dominated by hydrogen recombin…

astro-ph2006★ 2 cited

Dark Supergiant: Chandra's Limits on X-rays from Betelgeuse

Jennifer Posson-Brown, Vinay L. Kashyap, Deron O. Pease +1

We have analyzed Chandra calibration observations of Betelgeuse (alpha Ori, M2Iab, m_V=0.58, 131 pc) obtained at the aimpoint locations of the HRC-I (8 ks), HRC-S (8 ks), and ACIS-…

astro-ph2006★ 15 cited

Soft X-ray emission lines of Fe XV in solar flare observations and the Chandra spectrum of Capella

F. P. Keenan, J. J. Drake, S. Chung +5

Recent calculations of atomic data for Fe XV have been used to generate theoretical line ratios involving n = 3-4 transitions in the soft X-ray spectral region (52-83 A), for a wid…