Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für extraterrestrische Physik     Collection: Theory & Complex Plasmas     Display Documents



  history
ID: 5979.0, MPI für extraterrestrische Physik / Theory & Complex Plasmas
Toward a mass and radius determination of the nearby isolated neutron star RX J185635-3754
Authors:Pons, J. A.; Walter, F. M.; Lattimer, J. M.; Prakash, M.; Neuhäuser, R.; An, P. H.
Language:English
Date of Publication (YYYY-MM-DD):2002-01-10
Title of Journal:The Astrophysical Journal
Journal Abbrev.:Astrophys. J.
Volume:564
Issue / Number:2
Start Page:981
End Page:1006
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:We discuss efforts to determine the mass, radius, and surface composition of the nearby compact object RX J185635-3754 from its multiwavelength spectral energy distribution. We compute nonmagnetized model atmospheres and emergent spectra for selected compositions and gravities and discuss efforts to fit existing and new observational data from ROSAT, the Extreme Ultraviolet Explorer, and the Hubble Space Telescope. The spectral energy distribution matches that expected from a heavy-element-dominated atmosphere, but not from a uniform- temperature blackbody. Nonmagnetic light-element atmospheres cannot be simultaneously reconciled with the optical and X-ray data. We extend previous studies, which were limited to one fixed neutron star mass and radius. For uniform-temperature models dominated by heavy elements, the redshift z is constrained to be 0.3 less than or similar to z less than or similar to 0.4 and the best-fit mass and radius are Mapproximate to0.9 M-. and Rapproximate to6 km (for a 61 pc distance). These values for M and R together are not permitted for any plausible equation of state, including that of a self- bound strange quark star. A simplified two-temperature model allows masses and radii up to about 50% larger, or a factor of 2 in the case of a blackbody. The observed luminosity is consistent with the thermal emission of an isolated neutron star no older than about 10(6) yr, the age inferred from available proper motion and parallax information.
Free Keywords:dense matter; stars : fundamental parameters; stars : individual (RX J185635-3754); stars : neutron
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für extraterrestrische Physik
External Affiliations:SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA; SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA; Univ Roma La Sapienza, Dipartimento Fis G Marconi, I-00185 Rome, Italy; Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
Identifiers:ISI:000173166900042
ISSN:0004-637X
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.