The X-ray sources at the center of G266.1-1.2
| dc.creator | Mereghetti, S. | |
| dc.creator | Pellizzoni, A. | |
| dc.creator | De Luca, A. | |
| dc.date | 2001-12-06 | |
| dc.date.accessioned | 2026-07-07T02:01:43Z | |
| dc.date.available | 2026-07-07T02:01:43Z | |
| dc.description | We present optical observations of the fields of two X-ray sources located near the center of the shell-like supernova remnant G266.1-1.2. No objects brighter than R~22.5 and B~23 are present within the small Chandra error region of AX J0851.9-4617.4, besides a R~17 star that has already been excluded as a possible counterpart. A bright diffuse H_alpha nebula is present close to the position of the candidate neutron star. | |
| dc.description | 4 pages, latex, 3 figures, to appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P. O. Slane and B. M. Gaensler | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0112152 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0112152 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3854 | |
| dc.subject | Astrophysics | |
| dc.title | The X-ray sources at the center of G266.1-1.2 | |
| dc.type | text |