IAFE 05512
INSTITUTO DE ASTRONOMIA Y FISICA DEL ESPACIO
Unidad Ejecutora - UE
congresos y reuniones científicas
Título:
The interstellar medium towards the supernova remnant G24.7+0.6
Autor/es:
A. PETRIELLA, S. PARON, E. GIACANI
Lugar:
San Juan, Argentina
Reunión:
Congreso; 51 Reunión Anual de la Asociación Argentina de Astronomía; 2008
Institución organizadora:
AAA
Resumen:
We have carried out a study of the distribution and kinematics of the13CO J=1--0 line in the direction of the Galactic supernova remnant (SNR) G24.7+0.6.We find three molecular features: a ``molecular arm´´ and two molecular clouds, that present morphological correspondences with the radio continuum emission of the SNR. One of these clouds shows spectral kinematical evidences of perturbed molecular gas, maybe due to the action of SNR shock front. Thus, we suggest a possible physical association between the SNR and the molecular gas and we derive a distance of 3.5 kpc for G24.7+0.6.
