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the claim

Neutron stars are real astronomical objects confirmed by pulsar observations since 1967.

the verdict
SUPPORTED
the evidence backs this
Recorded sources
11 sources for · 0 against

Counts group repeated records of the same source within each side. They do not measure evidence strength or source independence.

Is it true that neutron stars are real astronomical objects confirmed by pulsar observations since 1967?

Yes. One peer-reviewed source explicitly states neutron stars were not recognized until pulsars were discovered in 1967, and another peer-reviewed source says pulsars discovered in 1967 were identified as neutron stars. Other sources treat neutron stars as real observed objects but do not address the 1967 pulsar confirmation.

Verdict: SUPPORTED · 11 sources for, 0 against · Last checked

The private library was unavailable for some searches in this check. Missing library results are not evidence against the claim.

Evidence for · 11
Neutron Stars and the Discovery of Pulsars.
1985
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George, G. (1985). Neutron Stars and the Discovery of Pulsars.. eric.ed.gov. https://eric.ed.gov/?id=EJ321614

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More for · 10
Why do some neutron stars become pulsars?
2015
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Why do some neutron stars become pulsars?. (2015). astronomy.stackexchange.com. https://astronomy.stackexchange.com/questions/11386/why-do-some-neutron-stars-become-pulsars

Neutron stars colliding with binary companions: formation of hypervelocity stars, pulsar planets, bumpy superluminous supernovae and Thorne–Żytkow objects
2022
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Hirai, R. & Podsiadlowski, P. (2022). Neutron stars colliding with binary companions: formation of hypervelocity stars, pulsar planets, bumpy superluminous supernovae and Thorne–Żytkow objects. doi.org. https://doi.org/10.1093/mnras/stac3007

Pulsar - Wikipedia
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Pulsar - Wikipedia. (n.d.). en.wikipedia.org. https://en.wikipedia.org/wiki/Pulsar

So Few Pulsars, So Few Females
2004
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So Few Pulsars, So Few Females. (2004). doi.org. https://doi.org/10.1126/science.304.5670.489

Neutron stars: A star powered by magnetism
1998
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R., K. S. & Christopher, T. (1998). Neutron stars: A star powered by magnetism. authors.library.caltech.edu. https://authors.library.caltech.edu/records/5kjq2-6bn70

Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
2020
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Philippe, L., Reed, E., & Katerina, C. (2020). Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations. authors.library.caltech.edu. https://doi.org/10.1103/physrevd.101.123007

STRUCTURE AND COMPOSITION OF NEUTRON STARS
2023
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A., G. & D., N. (2023). STRUCTURE AND COMPOSITION OF NEUTRON STARS. zenodo.org. https://doi.org/10.5281/zenodo.10117477

Interplay of astrophysics and nuclear physics in determining the properties of neutron stars
2025
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Jacob, G., Isaac, L., & Katerina, C. (2025). Interplay of astrophysics and nuclear physics in determining the properties of neutron stars. authors.library.caltech.edu. https://doi.org/10.1103/physrevd.111.023029

The emission of interpulses by a 6.45-h-period coherent radio transient
2025
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J., L. Y. W., M., C., & Tara, M. (2025). The emission of interpulses by a 6.45-h-period coherent radio transient. authors.library.caltech.edu. https://doi.org/10.1038/s41550-024-02452-z

A particle simulation for the global pulsar magnetosphere: the pulsar wind linked to the outer gaps
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A particle simulation for the global pulsar magnetosphere: the pulsar wind linked to the outer gaps. (n.d.). cir.nii.ac.jp. https://doi.org/10.1111/j.1365-2966.2007.11440.x

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