A Smoking Gun in the Carina Nebula

TL;DR

This paper reports the discovery of a neutron star in the Carina Nebula, indicating multiple star formation episodes and providing insights into the nebula's complex star formation history.

Contribution

It presents the first identification of a neutron star in the Carina Nebula, challenging existing theories about the nebula's star formation timeline.

Findings

Discovered a persistent X-ray source consistent with a neutron star.

Evidence suggests at least two major star formation episodes in the nebula.

Neutron star may explain high-energy phenomena observed in the region.

Abstract

The Carina Nebula is one of the youngest, most active sites of massive star formation in our Galaxy. In this nebula, we have discovered a bright X-ray source that has persisted for ~30 years. The soft X-ray spectrum, consistent with kT ~128 eV blackbody radiation with mild extinction, and no counterpart in the near- and mid-infrared wavelengths indicate that it is a ~1e6-year-old neutron star housed in the Carina Nebula. Current star formation theory does not suggest that the progenitor of the neutron star and massive stars in the Carina Nebula, in particular Eta Carinae, are coeval. This result suggests that the Carina Nebula experienced at least two major episodes of massive star formation. The neutron star may be responsible for remnants of high energy activity seen in multiple wavelengths.