The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

VF Suleimanov, J Poutanen, J Nättilä… - Monthly Notices of …, 2017 - academic.oup.com
Determining neutron star (NS) radii and masses can help to understand the properties of
matter at supra-nuclear densities. Thermal emission during thermonuclear X-ray bursts from …
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[引用][C] The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

VF Suleimanov, J Poutanen, J Nattila… - Monthly Notices of …, 2017 - ub01.uni-tuebingen.de
The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and
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The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

VF Suleimanov, J Poutanen, J Nättilä… - Mon. Not. Roy. Astron …, 2017 - inspirehep.net
Determining neutron star (NS) radii and masses can help to understand the properties of
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The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

VF Suleimanov, J Poutanen, J Nättilä… - arXiv preprint arXiv …, 2016 - arxiv.org
Determining neutron star (NS) radii and masses can help to understand the properties of
matter at supra-nuclear densities. Thermal emission during thermonuclear X-ray bursts from …

The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

V Suleimanov, J Nättilä, K Werner, M Revnivtsev… - dspace.kpfu.ru
Электронный архив КФУ :: The direct cooling tail method for X-ray burst analysis to constrain
neutron star masses and radii Электронный архив The direct cooling tail method for X-ray …

The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

VF Suleimanov, J Poutanen, J Nättilä… - Monthly Notices of …, 2017 - ui.adsabs.harvard.edu
Determining neutron star (NS) radii and masses can help to understand the properties of
matter at supra-nuclear densities. Thermal emission during thermonuclear X-ray bursts from …

The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

VF Suleimanov, J Poutanen, J Nättilä… - Monthly notices of the …, 2017 - diva-portal.org
Determining neutron star (NS) radii and masses can help to understand the properties of
matter at supra-nuclear densities. Thermal emission during thermonuclear X-ray bursts from …

[引用][C] The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

VF Suleimanov, J Poutanen… - … Notices of The …, 2017 - tobias-lib.ub.uni-tuebingen.de
The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and
radii The direct cooling tail method for X-ray burst analysis to constrain neutron star masses …

[引用][C] The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

V Suleimanov, J Poutanen, J Nättilä… - … -2017-466-1 …, 2017 - openrepository.ru
The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii
- «Национальный агрегатор открытых репозиториев российских университетов» (НОРА) …

[引用][C] The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

VF Suleimanov, J Poutanen, J Nättilä… - Monthly Notices of the …, 2016 - cir.nii.ac.jp
The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and
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