SIMBAD references

2001ApJ...548L.213M - Astrophys. J., 548, L213-L216 (2001/February-3)

The X-ray sources at the center of the supernova remnant RX J0852.0-4622.

MEREGHETTI S.

Abstract (from CDS):

We present a BeppoSAX observation of the X-ray source AX J0851.9-4617.4. This source has been proposed as the neutron star that is associated with the shell-like supernova remnant RX J0852.0-4622. At E>5 keV, the image shows the presence of a new source, SAX J0852.0-4615, that was not resolved from AX J0851.9-4617.4 in previous observations. The improved positional accuracy obtained for AX J0851.9-4617.4, along with its soft thermal spectrum (kT∼1.3 keV), confirms its possible identification with an early-type star. SAX J0852.0-4615, with its harder X-ray spectrum and higher X-ray-to-optical flux ratio, is a more likely candidate for the neutron star associated with the supernova remnant.

Abstract Copyright:

Journal keyword(s): ISM: Individual: Alphanumeric: G266.2-1.2 - Stars: Neutron - ISM: Supernova Remnants - X-Rays: Individual: Alphanumeric: RX J0851.9-4617.4 - X-Rays: Individual: Alphanumeric: RX J0852.0-4622

Nomenclature: [M2001b] JHHMMSS+DDMMSS N=1.

Simbad objects: 10

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2023.02.09-00:35:43

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