activity
20082014
most citedA catalogue of young runaway Hipparcos stars within 3kpc from the Sun

292 citations · 698 across the 21 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2014★ 17 cited

The Origin of the Young Pulsar PSR J0826+2637 and Its Possible Former Companion HIP 13962

N. Tetzlaff, B. Dincel, R. Neuhaeuser +1

We aim to identify the birth place of the young pulsar PSR J0826+2637 in order to determine its kinematic age and give constraints on its radial and spatial (kick) velocity. Since…

astro-ph.GA2012★ 7 cited

Is there a compact companion orbiting the late O-type binary star HD 164816?

L. Trepl, V. V. Hambaryan, T. Pribulla +7

We present a multi-wavelength (X-ray, -ray, optical and radio) study of HD 194816, a late O-type X-ray detected spectroscopic binary. X-ray spectra are analyzed and the X-ray ph…

astro-ph.GA2012★ 30 cited

Neutron stars from young nearby associations the origin of RXJ1605.3+3249

Nina Tetzlaff, Janos G. Schmidt, Markus M. Hohle +1

Many neutron stars (NSs) and runaway stars apparently come from the same regions on the sky. This suggests that they share the same birth places, namely associations and clusters o…

astro-ph.GA2011★ 58 cited

The origin of RXJ1856.5-3754 and RXJ0720.4-3125 -- updated using new parallax measurements

Nina Tetzlaff, Thomas Eisenbeiss, Ralph Neuhaeuser +1

RXJ1856 and RXJ0720 are the only young isolated radio-quiet neutron stars (NSs) for which trigonometric parallaxes were measured. Due to detection of their thermal emission in X-ra…

astro-ph.GA2010★ 292 cited

A catalogue of young runaway Hipparcos stars within 3kpc from the Sun

N. Tetzlaff, R. Neuhäuser, M. M. Hohle

Traditionally runaway stars are O and B type stars with large peculiar velocities.We want to extend this definition to young stars (up to ~50 Myr) of any spectral type and identify…

astro-ph.GA2009★ 11 cited

The origin of the Guitar pulsar

Nina Tetzlaff, Ralph Neuhaeuser, Markus M. Hohle

Among a sample of 140 OB associations and clusters, we want to identify probable parent associations for the Guitar pulsar (PSR B2224+65) which would then also constrain its age. F…