NASA telescope revealed the hidden properties of X-ray Pulsar RX J0032.9-7348

Pulsar neutron stars move rapidly, which emit electromagnetic radiation in various wavelengths including radio waves, optical, X-rays and gamma-rays. RX J0032.9-7348 has been classified as an X-ray pulsation as an X-ray pulsation as an X-ray transient source in the small Magalanic cloud (SMC) about 30 years ago. Nustar.

Search and observation campaign

According For the handbook of X-ray and gamma ray astrophysics, the Extraction-Paurd X-ray Pulsar (XRP) is neutron stars within the binary system that emit X-rays in regular pulses, operating by the enhancement of a substance from a fellow star. However, although the RX J0032.9-7348 has been known for decades, its properties are very rarely known and its optical equivalent has not been identified. Therefore, a team of astronomers led by Birendra Chhotare of Physical Research Laboratory (PRL) in Ahmedabad, India decided to take a close look at this Pulsar with Nussar and Nicher.
Dr. Chhotrai and his team were able to verify the X-ray Pulsation period of RX J0032.9-7348 through their comments and also discovered that this Pulsar has a double-pulses in a wide energy range, with small changes as energy dependence.

conclusion

Results of observation campaign, Published On the Arxiv Preprint server, the spin of this Pulsar gives the insight of dynamics and luminosity. The granular processes during the X-ray brighting phase increase its angular speed. It results in a spin -up of about -0,00033 seconds per day.
Pulsar’s brightness during the monitoring campaign varies from 8.2 undcillion to 37 Undecillion Erg/s. Researchers report that no evidence of iron emission line or cyclotron resonance was found in the energy spectrum of this source.