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arXiv:1909.08847v2 [astro-ph.HE] 9 Feb 2020

https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

An electrical switch based on Ag-tetracyanoquinodimethane ...

https://aip.scitation.org/doi/10.1063/1.2988272

de W Zhou · 2008 · Cité 16 fois — (b) A Ti∕Au film was thermally evaporated to connect the nanotube shown in (a) into ... containing tetrabutylammonium hexafluorophosphate (Bu4NPF6, 0.1M).

Multi-modal and multi-scale clinical retinal imaging system ...

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9187716/

de MF Shirazi · 2022 · Cité 2 fois — Figure 4f,h are the enlarged view (× 4) of photoreceptor cone mosaic ... FT fixation target, GS guide star, PC polarization controller, ...

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

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https://arxiv.org/pdf/1909.08847

de P Feola · 2019 · Cité 21 fois — The mass-radius relation for neutron stars in f(R) = R + αR2 gravity: a comparison ... This model is specially suitable to account for cos-.

Publications - STAR RESEARCH GROUP

https://www.starresearchgroup.com/publications.html

G. Peng, X. Xu*, F. Mei, G. Xu, J. Wu, D. Gao, J. E. Ellis, Y. Zhao, Y. Xing, ... G. V. Shurin, A. R. Murray, H. D. Leonard, J. S. Reynolds, D. W. Gutkin, ...

A Dynamical Gravitational Wave Source in a Dense Cluster

https://www.cambridge.org/core/journals/publications-of-the-astronomical-society-of-australia/article/dynamical-gravitational-wave-source-in-a-dense-cluster/72A34A9F855F9EB33E1708C4C96581A8

de JR Hurley · 2016 · Cité 34 fois — The peak central density of the new model is about 10 6stars pc −3 which is ... C. L., Ruiter, A., Valsecchi, F., Vink, J. S., & Hurley, J. R. 2010, ApJ, ...

JavaScript packages index - S | Snyk Open Source Advisor

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popular a b c d e f g h i j k l m n o p q r s t u v w x y z. Popular JavaScript Packages Index. sse.js · sse-pubsub · sset · ssf · ss-group-datatable · ssh2 ...

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a measurement at 400 nm using dark cloud shadow

https://academic.oup.com/mnras/article/470/2/2152/3854796

de K Mattila · 2017 · Cité 42 fois — For the cloud, and even for its dark core, we have to take into account a ... where fsca(τcl) is the fraction of scattered EBL from the dark cloud and.

LETTERS - Nature

https://www.nature.com/articles/289568a0.pdf

de S Danaher · 1981 · Cité 112 fois — f. Immun. 115,1617-1624 (1975). 35. Brugge, J. S. & Erikson, R. L. Nature 269, 346-348 (1977) ...

D. F. Figer's research works | Rochester Institute of ...

https://www.researchgate.net/scientific-contributions/D-F-Figer-13731164

If you are this author, and you don't want us to display this page ... formed clusters having a very high stellar density, as high as 106 stars pc-3.

is there evidence for flat cores in the halos of dwarf galaxies ...

http://iopscience.iop.org/0004-637X/657/2/773/pdf/63754.web.pdf

de O Valenzuela · 2007 · Cité 152 fois — present our hydrodynamical models of a dwarf galaxy and com- ... Maximum resolution (2 ; star) (pc).............. 60 ... F(x) ln (1 ю x) А x=(1 ю x);.

The effect of binaries on the dynamical mass determination of ...

https://www.aanda.org/articles/aa/full/2008/10/aa8897-07/aa8897-07.right.html

de MBN Kouwenhoven · 2008 · Cité 71 fois — 107 stars pc-3), binaries do not affect the dynamical mass estimation significantly ... a flat mass ratio distribution fq(q) = 1, and a thermal eccentricity ...

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JSC FCU Mobile for PC / Mac / Windows 7.8.10 - Napkforpc.com

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