@inproceedings{acae516c3f3843ea93ff3a99465cc014,
title = "X-ray properties of G308.3-1.4 and its central compact object",
abstract = "We present a short Chandra observation that confirms a previous unidentified extended X-ray source, G308.3-1.4, as a new supernova remnant (SNR) in the Milky Way. Apart from identifying its SNR nature, a bright X-ray point source has also been discovered at the geometrical center. Its X-ray spectral properties are similar to those of a particular class of neutron star known as central compact objects (CCOs). On the other hand, the optical properties of this counterpart suggests it to be a late-type star. Together with the interesting ∼ 1.4 hours X-ray periodicity found by Chandra, this system can possibly provide the first direct evidence of a compact binary survived in a supernova explosion.",
keywords = "X-rays, supernova remnants",
author = "Seo, \{K. A.\} and Hui, \{C. Y.\} and Huang, \{R. H.H.\} and L. Trepl and Lu, \{T. N.\} and Kong, \{A. K.H.\} and Walter, \{F. M.\}",
year = "2012",
month = aug,
doi = "10.1017/S1743921312024611",
language = "English",
isbn = "9781107033801",
series = "Proceedings of the International Astronomical Union",
number = "S291",
pages = "489--491",
editor = "\{Van Leeuwen\}, Joeri",
booktitle = "Neutron Stars and Pulsars",
edition = "S291",
}