Near-Infrared and Optical Limits for the Central X-ray Point Source in the Cassiopeia A Supernova Remnant
arXiv:astro-ph/0509552 · doi:10.1086/498087
Abstract
Near-infrared images of the center of the Cas A supernova remnant taken with the NICMOS 2 camera on HST using the F110W and F160W filters (~J & ~H bands) have magnitude limits of 26.2 and 24.6 respectively, but reveal no sources within a 1.2" radius of the Chandra detected central X-ray point source (XPS). The NICMOS data, taken together with broadband optical magnitude limits (R ~ 28 mag) obtained from a deep STIS CCD exposure taken with a clear filter (50CCD), indicate that the XPS luminosities are very low in the optical/NIR bands (e.g., L_H < 3 x E29 erg/s) with no optical, J, or H band counterpart to the XPS easily detectable by HST. We discuss the nature of the Cas A central compact object based upon these new near-infrared and optical flux limits.
14 pages including 6 tables and 3 figures. To appear in the Astrophysical Journal
References in corpus (13)
- A Million-Second Chandra View of Cassiopeia A
- XMM-Newton observations of the supernova remnant RX J1713.7-3946 and its central source
- Infrared Echoes near the Supernova Remnant Cassiopeia A
- XMM-Newton observations of the Galactic Supernova Remnant CTB 109 (G109.1-1.0)
- Discovery of a 105 ms X-ray Pulsar in Kesteven 79: On the Nature of Compact Central Objects in Supernova Remnants
- Correlated Infrared and X-ray Flux Changes Following the 2002 June Outburst of the Anomalous X-ray Pulsar 1E 2259+586
- Where Are All The Fallback Disks? Constraints on Propeller Systems
- Precise Localization of the Soft Gamma Repeater SGR 1627-41 and the Anomalous X-ray Pulsar AXP 1E1841-045 with Chandra
- Infrared and X-ray variability of the transient Anomalous X-ray Pulsar XTE J1810-197
- The Broad-Band Spectrum and Infrared Variability of the Magnetar AXP 1E1048.1-5937
- X-Ray Timing, Spectroscopy and Photometry of the Anomalous X-Ray Pulsar Candidate CXOU J010043.1-721134
- A Deep Infrared Search for AXP 1E 1841-045
- Possible Optical Detection of the Anomalous X-ray Pulsar CXOU J010043.1-721134
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- Searching for gravitational waves from Cassiopeia A with LIGO
- Direct Confirmation of the Asymmetry of the Cas A Supernova with Light Echoes
- Magnetic Phases in Three-Flavor Color Superconductivity
- AKARI and BLAST Observations of the Cassiopeia A Supernova Remnant and Surrounding Interstellar Medium
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- A dedicated Chandra ACIS observation of the central compact object in the Cassiopeia A supernova remnant
- Small-Scale X-ray Variability in the Cassiopeia A Supernova Remnant
- A JWST Survey of the Supernova Remnant Cassiopeia A
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- Deep infrared observations of the puzzling central X-ray source in RCW103
- No surviving stellar companion for Cassiopeia A
- Optical and Infrared Observations of the X-ray source 1WGA J1713.43949 in the G347.3-0.5 SNR
- Near Infrared Counterpart of 2E 1613.5-5053, the Central Source in Supernova Remnant RCW 103
- HST and VLT observations of the neutron star 1E 1207.4-5209
- VLT observations of the Central Compact Object in the Vela Jr. supernova remnant
- An X-ray study of the SNR G344.7-0.1 and the central object CXOU J170357.8-414302
- What causes the absence of pulsations in Central Compact Objects in Supernova Remnants?
- Evidence for a Binary Companion to the Central Compact Object 1E 1207.4-5209
- Searching for Debris Disks around Isolated Pulsars
- Hints of a second explosion (a quark nova) in Cassiopeia A Supernova
- An X-ray upper limit on the presence of a Neutron Star for the Small Magellanic Cloud and Supernova Remnant 1E0102.2-7219