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On the implications of the radio and X-ray pulsar in the Supernova Remnant MSH 15-52

G. Srinivasan, K. S. Dwarakanath, V. Radhakrishnan

Open publisher page 6 citations

Abstract

Comparison of the X-ray nebulosity surrounding the X-ray and radio pulsar in the shell-type SNR MSH 15-52 with the Crab nebula leads to an initial period for the pulsar ~ 70 ms. The association of the pulsar with the shell remnant confirms the validity of the ∑-t approach in determining the ages of young SNRs using historical calibrators.

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What this paper is about

Comparison of the X-ray nebulosity surrounding the X-ray and radio pulsar in the shell-type SNR MSH 15-52 with the Crab nebula leads to an initial period for the pulsar ~ 70 ms. The association of the pulsar with the shell remnant confirms the validity of the ∑-t approach in determining the ages of young SNRs using historical calibrators.

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OpenAlex reports 6 citations for this work. Citation counts describe recorded attention and do not establish research quality.

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Available abstract

Comparison of the X-ray nebulosity surrounding the X-ray and radio pulsar in the shell-type SNR MSH 15-52 with the Crab nebula leads to an initial period for the pulsar ~ 70 ms. The association of the pulsar with the shell remnant confirms the validity of the ∑-t approach in determining the ages of young SNRs using historical calibrators.

Key concepts: Pulsar, Supernova remnant, Physics, Astrophysics, Nebula, Crab Nebula, Supernova, Astronomy

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