activity
19962021
most citedRadio emission from Supernova Remnants

166 citations · 1.1k across the 42 of their papers we have counts for

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astro-ph2008★ 30 cited

High resolution radio study of the Pulsar Wind Nebula within the Supernova Remnant G0.9+0.1

Gloria Dubner, Elsa Giacani, Anne Decourchelle

We have conducted a radio study at 3.6, 6 and 20 cm using ATCA and VLA and reprocessed XMM-Newton and Chandra data of the pulsar wind nebula (PWN) in the supernova remnant (SNR) G0…

astro-ph2008★ 29 cited

Isolated X-ray -- infrared sources in the region of interaction of the supernova remnant IC 443 with a molecular cloud

A. M. Bykov, A. M. Krassilchtchikov, Yu. A. Uvarov +5

The nature of the extended hard X-ray source XMMU J061804.3+222732 and its surroundings is investigated using XMM-Newton, Chandra, and Spitzer observations. This source is located…

astro-ph2006★ 5 cited

On the nature of the hard X-ray source IGR J2018+4043

A. M. Bykov, A. M. Krassilchtchikov, Yu. A. Uvarov +13

We found a very likely counterpart to the recently discovered hard X-ray source IGR J2018+4043 in the multi-wavelength observations of the source field. The source, originally disc…

astro-ph2005★ 21 cited

The interior of the SNR RX J0852.0-4622 (Vela Jr) at radio wavelengths

E. M. Reynoso, G. Dubner, E. Giacani +2

Aim: We observed the center of the supernova remnant Vela Jr in radio continuum in order to search for a counterpart to the compact central X-ray source CXOU J085201.4-461753, poss…

astro-ph2005

Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1

E. Giacani, N. Loiseau, G. Dubner +1

We report on new VLA radio and XMM-Newton X-ray observations of the SNR G352.7-0.1. These high sensitivity, high resolution data reveal that G352.7-0.1 belongs to the thermal compo…

astro-ph2004★ 5 cited

The neutral gas in the environs of the Geminga gamma-ray pulsar

E. Giacani, E. Reynoso, G. Dubner +3

We present a high-resolution (24 arcsec) study of the HI interstellar gas distribution around the radio-quiet neutron star Geminga. Based on Very Large Array (VLA) and MPIfR Effels…