We analize the 12CO emission towards the brightest X-ray knot in the supernova remnant (SNR) Puppis A. The observations were performed with the SEST telescope in the 12CO J=1--0 and 2--1 lines (beams of 45" and 23" respectively). We discovered a compact molecular clump near the radio and X-ray maxima and calculated its physical parameters. From the comparison with Chandra X-ray data we conclude that this molecular clump lies in front of Puppis A along the line of sight. The possibilities of a recent interaction between the SNR and the molecular gas are analyzed.Se analiza la emisión del 12CO en la región más brillante de emisión de rayos X del remanente de supernova (RSN) Puppis A. Las observaciones fueron realizadas en las transiciones J=1...
International audienceSupernova remnants (SNRs) are the best candidates for galactic cosmic ray acce...
RCW 103 is a shell type supernova remnant (SNR) that, according to near infrared observations, is in...
Most supernova remnants (SNRs) in our Galaxy are expected to be close to their parent molecular clou...
We analize the 12CO emission towards the brightest X-ray knot in the supernova remnant (SNR) Puppis ...
Aims. With the purpose of producing the first detailed full view of Puppis A in X-rays, we carried o...
We have carried out a study of the interstellar medium (ISM) toward a shell-like supernova remnant S...
Aims.This paper reports molecular observations towards the bright eastern knot (BEK) in the SNR Pupp...
Aims. This paper reports molecular observations towards the Bright Eastern Knot (BEK) in the SNR Pu...
Aims.This paper reports molecular observations towards the bright eastern knot (BEK) in the SNR Pup...
In this paper we report on a new study of the SNR Puppis A based on VLA observations at 1425 MHz; th...
Aims. We report results of an X-ray study of the supernova remnant (SNR) G344.7-0.1 and the point-li...
Aims. HESS J1858+020 is a weak γ-ray source lying near the southern border of the SNR G35.6-0.4. A m...
We introduce a distinct method to perform spatially-resolved spectral analysis of astronomical sourc...
We report INTEGRAL IBIS γ-ray and VLA radio observations of G0.570-0.018, a diffuse X-ray source re...
Aims. The eastern border of the SNR G18.8+0.3, close to an HII regions complex, is a very interestin...
International audienceSupernova remnants (SNRs) are the best candidates for galactic cosmic ray acce...
RCW 103 is a shell type supernova remnant (SNR) that, according to near infrared observations, is in...
Most supernova remnants (SNRs) in our Galaxy are expected to be close to their parent molecular clou...
We analize the 12CO emission towards the brightest X-ray knot in the supernova remnant (SNR) Puppis ...
Aims. With the purpose of producing the first detailed full view of Puppis A in X-rays, we carried o...
We have carried out a study of the interstellar medium (ISM) toward a shell-like supernova remnant S...
Aims.This paper reports molecular observations towards the bright eastern knot (BEK) in the SNR Pupp...
Aims. This paper reports molecular observations towards the Bright Eastern Knot (BEK) in the SNR Pu...
Aims.This paper reports molecular observations towards the bright eastern knot (BEK) in the SNR Pup...
In this paper we report on a new study of the SNR Puppis A based on VLA observations at 1425 MHz; th...
Aims. We report results of an X-ray study of the supernova remnant (SNR) G344.7-0.1 and the point-li...
Aims. HESS J1858+020 is a weak γ-ray source lying near the southern border of the SNR G35.6-0.4. A m...
We introduce a distinct method to perform spatially-resolved spectral analysis of astronomical sourc...
We report INTEGRAL IBIS γ-ray and VLA radio observations of G0.570-0.018, a diffuse X-ray source re...
Aims. The eastern border of the SNR G18.8+0.3, close to an HII regions complex, is a very interestin...
International audienceSupernova remnants (SNRs) are the best candidates for galactic cosmic ray acce...
RCW 103 is a shell type supernova remnant (SNR) that, according to near infrared observations, is in...
Most supernova remnants (SNRs) in our Galaxy are expected to be close to their parent molecular clou...