Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

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Compactness of Neutron Stars.Limits on thermal variations in a dozen quiescent neutron stars over a decade Lense-Thirring precession in ULXs as a possible means to constrain the neutron star equation of state TheNuSTARview of the non-thermal emission from PSR J0437−4715

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P2860

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

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http://www.wikidata.org/entity/Q57458765

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im August 2014 veröffentlichter wissenschaftlicher Artikel

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wetenschappelijk artikel

@nl

наукова стаття, опублікована в серпні 2014

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name

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

@en

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

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Item

label

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

@en

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

@nl

prefLabel

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

@en

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

@nl

P1476

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

@en

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A. M. Cool

http://www.w3.org/2001/XMLSchema#string

C. O. Heinke

http://www.w3.org/2001/XMLSchema#string

D. Haggard

http://www.w3.org/2001/XMLSchema#string

H. N. Cohn

http://www.w3.org/2001/XMLSchema#string

J. Anderson

http://www.w3.org/2001/XMLSchema#string

J. E. Grindlay

http://www.w3.org/2001/XMLSchema#string

N. A. Webb

http://www.w3.org/2001/XMLSchema#string

P. M. Lugger

http://www.w3.org/2001/XMLSchema#string

S. Bogdanov

http://www.w3.org/2001/XMLSchema#string

W. C. G. Ho

http://www.w3.org/2001/XMLSchema#string

P2860

Age estimates of globular clusters in the Milky Way: constraints on cosmology

A catalog of parameters for globular clusters in the Milky Way

Solar System Abundances and Condensation Temperatures of the Elements

A neutron star with a carbon atmosphere in the Cassiopeia A supernova remnant.

A radio pulsar/x-ray binary link.

Swings between rotation and accretion power in a binary millisecond pulsar.

An age difference of two billion years between a metal-rich and a metal-poor globular cluster.

The Chemical Composition of the Sun

The dynamical distance and intrinsic structure of the globular cluster ω Centauri

The European Photon Imaging Camera on XMM-Newton: The pn-CCD camera

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443–456

http://www.w3.org/2001/XMLSchema#string

P31

scholarly article

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10.1093/MNRAS/STU1449

http://www.w3.org/2001/XMLSchema#string

P407

English

P433

http://www.w3.org/2001/XMLSchema#string

P478

444

http://www.w3.org/2001/XMLSchema#string

P50

Sergio Campana

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2014-08-16T00:00:00Z

http://www.w3.org/2001/XMLSchema#dateTime

P818

1406.1497

http://www.w3.org/2001/XMLSchema#string

P819

2014MNRAS.444..443H

http://www.w3.org/2001/XMLSchema#string

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

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P2860

P2860

Improved mass and radius constraints for quiescent neutron stars in ω Cen and NGC 6397

description

name

type

label

prefLabel

P1433

P1476

P2093

P2860

P304

P31

P356

P407

P433

P478

P50

P577

P818

P819

P356

P1433

P1476

P2093

P2860

P304

P31

P356

P407

P433

P478

P50

P577

P818

P819