Indication of a Pulsar Wind Nebula in the Hard X-Ray Emission from SN 1987A

@article{Greco2021IndicationOA,
  title={Indication of a Pulsar Wind Nebula in the Hard X-Ray Emission from SN 1987A},
  author={Emanuele Greco and Marco Miceli and Salvatore Orlando and Barbara Olmi and Fabrizio Bocchino and Shigehiro Nagataki and Masaomi Ono and Akira Dohi and Giovanni Peres},
  journal={The Astrophysical Journal Letters},
  year={2021},
  volume={908}
}
Since the day of its explosion, SN 1987A (SN87A) was closely monitored with the aim to study its evolution and to detect its central compact relic. The detection of neutrinos from the supernova strongly supports the formation of a neutron star (NS). However, the constant and fruitless search for this object has led to different hypotheses on its nature. To date, the detection in the Atacama Large Millimeter/submillimeter Array data of a feature that is somehow compatible with the emission… 

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