Zobrazeno 1 - 10
of 1 092
pro vyhledávání: '"Link B"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Haveman, R.A., Bäumlein, M., van Veelen, N., Oberkircher, L., Beeres, F.J.P., Babst, R., Ruchholtz, S., Link, B-C.
Publikováno v:
In Injury December 2022 53(12):4062-4066
Autor:
Arzoumanian, Z., Bogdanov, S., Cordes, J., Gendreau, K., Lai, D., Lattimer, J., Link, B., Lommen, A., Miller, C., Ray, P., Rutledge, R., Strohmayer, T., Wilson-Hodge, C., Wood, K.
The characteristic physical timescales near stellar-mass compact objects are measured in milliseconds. These timescales -- the free-fall time, the fastest stable orbital period, and stellar spin periods -- encode the fundamental physical properties o
Externí odkaz:
http://arxiv.org/abs/0902.3264
Autor:
Burgio, G. F., Link, B.
Publikováno v:
Nucl.Phys.Proc.Suppl.165:231-236,2007
Young, rapidly rotating neutron stars could accelerate protons to energies of $\sim 1$ PeV close to the stellar surface, which scatter with x-rays from the stellar surface through the $\Delta$ resonance and produce pions. The pions subsequently decay
Externí odkaz:
http://arxiv.org/abs/astro-ph/0609561
Publikováno v:
Phys.Rev.Lett.98:071101,2007
We show the existence of a strong trend between neutron star surface temperature and the dipolar component of the magnetic field extending through three orders of field magnitude, a range that includes magnetars, radio-quiet isolated neutron stars, a
Externí odkaz:
http://arxiv.org/abs/astro-ph/0607583
Publikováno v:
Mon.Not.Roy.Astron.Soc.Lett. 370 (2006) L76-L79
We present an analysis of the spin-down parameters for 131 radio pulsars for which $\ddot\nu$ has been well determined. These pulsars have characteristic ages ranging from $10^{3} - 10^{8}$ yr and spin periods in the range 0.4--30 s; nearly equal num
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605380
Autor:
Link, B., Burgio, Fiorella
Publikováno v:
Phys.Rev.Lett. 94 (2005) 181101
Neutron stars are efficient accelerators for bringing charges up to relativistic energies. We show that if positive ions are accelerated to ~1 PeV near the surface of a young neutron star (t_age < about 10^5 yr), protons interacting with the star's r
Externí odkaz:
http://arxiv.org/abs/astro-ph/0412520
Autor:
Link, B., Cutler, C.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 336 (2002) 211
The neutron vortices thought to exist in the inner crust of a neutron star interact with nuclei and are expected to pin to the nuclear lattice. Evidence for long-period precession in pulsars, however, requires that pinning be negligible. We estimate
Externí odkaz:
http://arxiv.org/abs/astro-ph/0108281
Publikováno v:
Phys.Rev.Lett.83:3362-3365,1999
With the aim of constraining the structural properties of neutron stars and the equation of state of dense matter, we study sudden spin-ups, glitches, occurring in the Vela pulsar and in six other pulsars. We present evidence that glitches represent
Externí odkaz:
http://arxiv.org/abs/astro-ph/9909146