File Download
There are no files associated with this item.
Links for fulltext
(May Require Subscription)
- Publisher Website: 10.1111/j.1365-2966.2006.11133.x
- Scopus: eid_2-s2.0-33845770255
- Find via
Supplementary
-
Citations:
- Scopus: 0
- Appears in Collections:
Article: Measuring neutron star mass and radius with three mass-radius relations
| Title | Measuring neutron star mass and radius with three mass-radius relations |
|---|---|
| Authors | |
| Keywords | Equation of state Pulsars: general Stars: neutron X-rays: stars |
| Issue Date | 2007 |
| Citation | Monthly Notices of the Royal Astronomical Society, 2007, v. 374, n. 1, p. 232-236 How to Cite? |
| Abstract | We propose to determine the mass and radius of a neutron star (NS) using three measurable mass-radius relationships, namely the 'apparent' radius inferred from the NS thermal emission, the gravitational redshift inferred from the absorption lines, as well as the averaged stellar mass density inferred from the orbital Keplerian frequency derived from the kilohertz quasi-periodic oscillation data. We apply the method to constrain the NS mass and radius of the X-ray sources, 1E 1207.4-5209, Aql X-1 and EXO 0748-676. © 2006 The Authors. |
| Persistent Identifier | http://hdl.handle.net/10722/361058 |
| ISSN | 2023 Impact Factor: 4.7 2023 SCImago Journal Rankings: 1.621 |
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Zhang, C. M. | - |
| dc.contributor.author | Yin, H. X. | - |
| dc.contributor.author | Kojima, Y. | - |
| dc.contributor.author | Chang, H. K. | - |
| dc.contributor.author | Xu, R. X. | - |
| dc.contributor.author | Li, X. D. | - |
| dc.contributor.author | Zhang, B. | - |
| dc.contributor.author | Kiziltan, B. | - |
| dc.date.accessioned | 2025-09-16T04:14:31Z | - |
| dc.date.available | 2025-09-16T04:14:31Z | - |
| dc.date.issued | 2007 | - |
| dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, 2007, v. 374, n. 1, p. 232-236 | - |
| dc.identifier.issn | 0035-8711 | - |
| dc.identifier.uri | http://hdl.handle.net/10722/361058 | - |
| dc.description.abstract | We propose to determine the mass and radius of a neutron star (NS) using three measurable mass-radius relationships, namely the 'apparent' radius inferred from the NS thermal emission, the gravitational redshift inferred from the absorption lines, as well as the averaged stellar mass density inferred from the orbital Keplerian frequency derived from the kilohertz quasi-periodic oscillation data. We apply the method to constrain the NS mass and radius of the X-ray sources, 1E 1207.4-5209, Aql X-1 and EXO 0748-676. © 2006 The Authors. | - |
| dc.language | eng | - |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | - |
| dc.subject | Equation of state | - |
| dc.subject | Pulsars: general | - |
| dc.subject | Stars: neutron | - |
| dc.subject | X-rays: stars | - |
| dc.title | Measuring neutron star mass and radius with three mass-radius relations | - |
| dc.type | Article | - |
| dc.description.nature | link_to_subscribed_fulltext | - |
| dc.identifier.doi | 10.1111/j.1365-2966.2006.11133.x | - |
| dc.identifier.scopus | eid_2-s2.0-33845770255 | - |
| dc.identifier.volume | 374 | - |
| dc.identifier.issue | 1 | - |
| dc.identifier.spage | 232 | - |
| dc.identifier.epage | 236 | - |
| dc.identifier.eissn | 1365-2966 | - |