115 citations · 727 across the 17 of their papers we have counts for
17 papers
DEM L241, a Supernova Remnant containing a High-Mass X-ray Binary
F. D. Seward, P. A. Charles, D. L. Foster +5
A Chandra observation of the Large Magellanic Cloud supernova remnant DEM L241 reveals an interior unresolved source which is probably an accretion-powered binary. The optical coun…
The Thermal Composite Supernova Remnant Kes 27 as Viewed by CHANDRA: Shock Reflection from a Cavity Wall
Yang Chen, Frederick D. Seward, Ming Sun +1
We present a spatially resolved spectroscopic study of the thermal composite supernova remnant Kes 27 with Chandra. The X-ray spectrum of Kes 27 is characterized by K lines from Mg…
X-ray Timing of PSR J1852+0040 in Kesteven 79: Evidence of Neutron Stars Weakly Magnetized at Birth
J. P. Halpern, E. V. Gotthelf, F. Camilo +1
The 105-ms X-ray pulsar J1852+0040 is the central compact object (CCO) in SNR Kes 79. We report a sensitive upper limit on its radio flux density of 12 uJy at 2 GHz using the NRAO…
Faint X-ray Structure in the Crab Pulsar-Wind Nebula
F. D. Seward, W. H. Tucker, R. A. Fesen
We report on a Chandra observation of the Crab Nebula that gives the first clear view of the faint boundary of the Crab's X-ray-emitting Pulsar Wind Nebula, or PWN. There is struct…
CHANDRA Observations of the X-ray Halo around the Crab Nebula
F. D. Seward, P. Gorenstein, R. K. Smith
Two Chandra observations have been used to search for thermal X-ray emission from within and around the Crab Nebula. Dead-time was minimized by excluding the brightest part of the…
Supernova Remnants in the Magellanic Clouds. V. The Complex Interior Structure of the N206 SNR
R. M. Williams, Y. -H. Chu, J. R. Dickel +4
The N206 supernova remnant (SNR) in the Large Magellanic Cloud (LMC) has long been considered a prototypical "mixed morphology" SNR. Recent observations, however, have added a new…