We have observed the H i distribution in an area 40 × 40 arcmin2 around the neutron star candidate RX J0822–4300, which is located in the supernova remnant Puppis A. The observations of the λ21-cm line were obtained with the Australia Telescope Compact Array and were combined with single-dish data from the Southern Galactic Plane Survey. The spatial resolution is 90 arcsec, and the velocity resolution is 1 km s−1. A sensitivity of ∼0.7 K was achieved. The results revealed a double-lobed feature of reduced emission at +16 km s−1, centred on the central compact object (CCO), and aligned with an H i hole blueshifted by 13 km s−1. The H i depressions have probably been created by the sweeping up of ∼2 M⊙. The alignment between the lobes and the...
By making use of the sub-arcsecond angular resolution of the High Resolution Camera (HRC-I) aboard t...
We have obtained the first high-dispersion observations of RX Pup in the wavelength region 1200-2000...
A detailed study of the distribution of 21-cm emission in the vicinity of the Orion Nebula shows the...
We have observed the H i distribution in an area 40 × 40 arcmin2 around the neutron star candidate R...
We have observed the HI distribution in an area 40' x 40' around the neutron star candidate RX J0822...
We observed the supernova remnant (SNR) Puppis A in the 21 cm line with the Australia Telescope Comp...
We observed the supernova remnant Puppis A in the 21 cm line with the Australia Telescope Compact Ar...
The distribution and kinematics of neutral hydrogen have been studied in a wide area around the supe...
Using the Australia Telescope Compact Array, we have carried out a survey of the H I emission in the...
We have investigated the neutral hydrogen in the direction of the Circinus OB1 association with part...
RX J0822-4300 is the central compact object associated with the Puppis A supernova remnant. Previous...
We analyse the distribution of the interstellar matter in the environs of the Wolf-Rayet star LSS 39...
The neutral hydrogen distribution has been studied in the direction of three Galactic Wolf-Rayet (WR...
Context. Massive stars deeply modify their surrounding interstellar medium (ISM) via their high thro...
We have investigated the neutral hydrogen in the direction of the Circinus OB1 association with part...
By making use of the sub-arcsecond angular resolution of the High Resolution Camera (HRC-I) aboard t...
We have obtained the first high-dispersion observations of RX Pup in the wavelength region 1200-2000...
A detailed study of the distribution of 21-cm emission in the vicinity of the Orion Nebula shows the...
We have observed the H i distribution in an area 40 × 40 arcmin2 around the neutron star candidate R...
We have observed the HI distribution in an area 40' x 40' around the neutron star candidate RX J0822...
We observed the supernova remnant (SNR) Puppis A in the 21 cm line with the Australia Telescope Comp...
We observed the supernova remnant Puppis A in the 21 cm line with the Australia Telescope Compact Ar...
The distribution and kinematics of neutral hydrogen have been studied in a wide area around the supe...
Using the Australia Telescope Compact Array, we have carried out a survey of the H I emission in the...
We have investigated the neutral hydrogen in the direction of the Circinus OB1 association with part...
RX J0822-4300 is the central compact object associated with the Puppis A supernova remnant. Previous...
We analyse the distribution of the interstellar matter in the environs of the Wolf-Rayet star LSS 39...
The neutral hydrogen distribution has been studied in the direction of three Galactic Wolf-Rayet (WR...
Context. Massive stars deeply modify their surrounding interstellar medium (ISM) via their high thro...
We have investigated the neutral hydrogen in the direction of the Circinus OB1 association with part...
By making use of the sub-arcsecond angular resolution of the High Resolution Camera (HRC-I) aboard t...
We have obtained the first high-dispersion observations of RX Pup in the wavelength region 1200-2000...
A detailed study of the distribution of 21-cm emission in the vicinity of the Orion Nebula shows the...