literature
Literature
Authors
Jobs
Seminars
Conferences
DataBETA

A New Young Galactic Supernova Remnant Containing a Compact Object: G15.9+0.2

Oct, 2006
4 pages
Published in:
  • Astrophys.J.Lett. 652 (2006) L45-L48
e-Print:
DOI:
View in:
pdf
reference search32 citations

Citations per year

2006201120162021202401234
Abstract: (arXiv)
We identify the radio-emitting shell-type supernova remnant G15.9+0.2 as a relatively young remnant containing an X-ray point source that may be its associated neutron star. The integrated spectrum of the remnant shell obtained from our 30 ks exploratory Chandra observation shows very strong lines that require elevated element abundances from ejecta, in particular of sulfur. A plane-shock model fit gives a temperature kT=0.9(0.8,1.0)kT = 0.9 (0.8, 1.0) keV, an ionization timescale net=6(4,9)×1010n_et = 6 (4, 9) \times 10^{10} cm−3^{-3} s, and a sulfur abundance of 2.1 (1.7, 2.7) times solar (90% confidence limits). Two-component models with one solar and one enriched component are also plausible, but are not well constrained by the data. Various estimates give a remnant age of order 10310^3 yr, which would make G15.9+0.2 among the dozen or so youngest remnants in the Galaxy. The sparse point source spectrum is consistent with either a steep Γ∼\Gamma \sim 4 power law or a kT∼kT \sim 0.4 keV blackbody. The spectrum is absorbed by a H column density NH∼4×1022N_H \sim 4 \times 10^{22} cm−2^{-2} similar to that required for the remnant shell. The implied 2--9.5 keV source luminosity is about 103310^{33} ergs s−1^{-1} for an assumed distance of 8.5 kpc consistent with the high absorption column. We suggest that the point source is either a rotation-powered pulsar or a compact central object (CCO).
  • ISM: individual (G15.9+0.2)
  • stars: neutron
  • supernova remnants
  • X-rays: general
  • X-rays: ISM