Add to ORKGNew results of HST and VLT observations of isolated pulsars and their environments are presented. We present the first deep optical observations of the nearby pulsar PSR J0108-1431, the identification evidence of PSR 1929+10 based on the proper motion measurement of its optical counterpart and a deep investigation at optical wavelengths of the X-ray PWN around the Vela pulsar
Context. The X-ray observations performed with the R\uf6ntgen Satellite (ROSAT) have led to the disc...
We report on the proper motion measurement of the proposed optical counterpart of the X-ray/radio pu...
International audienceWe report nondetections of the ∼3 × 108 yr old, slow, isolated, rotation-power...
We present the results of first deep optical observations of the field of the old ($\sim 10^8$ yr), ...
We report on deep VLT observations of the fields of two nearby, isolated millisecond pulsars, PSR J1...
Context. Optical-ultraviolet (UV) observations of > 100 Myr pulsars are crucial to understand the l...
We present optical data gathered by the VLT Test Camera in the V-band at the radio (interferometric)...
Context. Optical observations of pulsars are crucial to studying the neutron star properti...
Context. The launch of the Fermi Gamma-ray Space Telescope in 2008 opened new perspectives in the mu...
Context. The launch of the Fermi Gamma-ray Space Telescope in 2008 opened new perspectives in the mu...
Given their intrinsic faintness, isolated neutron stars represent an elusive target for optical astr...
Context. The multi-wavelength study of old (>100 Myr) radio pulsars holds the key to understanding t...
Context. The 535 kyear old radio pulsar B1055–52 is the oldest of the “Three Musketeers”, the group ...
Fields of Geminga, PSR B0950+08, PSR J1908+0734 and PSR J0108-1431 have been observed within the pro...
Context. The study of the younger, and brighter, pulsars is important for understanding the optical ...
Context. The X-ray observations performed with the R\uf6ntgen Satellite (ROSAT) have led to the disc...
We report on the proper motion measurement of the proposed optical counterpart of the X-ray/radio pu...
International audienceWe report nondetections of the ∼3 × 108 yr old, slow, isolated, rotation-power...
We present the results of first deep optical observations of the field of the old ($\sim 10^8$ yr), ...
We report on deep VLT observations of the fields of two nearby, isolated millisecond pulsars, PSR J1...
Context. Optical-ultraviolet (UV) observations of > 100 Myr pulsars are crucial to understand the l...
We present optical data gathered by the VLT Test Camera in the V-band at the radio (interferometric)...
Context. Optical observations of pulsars are crucial to studying the neutron star properti...
Context. The launch of the Fermi Gamma-ray Space Telescope in 2008 opened new perspectives in the mu...
Context. The launch of the Fermi Gamma-ray Space Telescope in 2008 opened new perspectives in the mu...
Given their intrinsic faintness, isolated neutron stars represent an elusive target for optical astr...
Context. The multi-wavelength study of old (>100 Myr) radio pulsars holds the key to understanding t...
Context. The 535 kyear old radio pulsar B1055–52 is the oldest of the “Three Musketeers”, the group ...
Fields of Geminga, PSR B0950+08, PSR J1908+0734 and PSR J0108-1431 have been observed within the pro...
Context. The study of the younger, and brighter, pulsars is important for understanding the optical ...
Context. The X-ray observations performed with the R\uf6ntgen Satellite (ROSAT) have led to the disc...
We report on the proper motion measurement of the proposed optical counterpart of the X-ray/radio pu...
International audienceWe report nondetections of the ∼3 × 108 yr old, slow, isolated, rotation-power...