SIMBAD references

2009ApJ...695L...4H - Astrophys. J., 695, L4-L9 (2009/April-2)

A smoking gun in the Carina nebula.

HAMAGUCHI K., CORCORAN M.F., EZOE Y., TOWNSLEY L., BROOS P., GRUENDL R., VAIDYA K., WHITE S.M., STROHMAYER T., PETRE R. and CHU Y.-H.

Abstract (from CDS):

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 indicates that it is a ∼106 year old neutron star housed in the Carina Nebula. Current star formation theory does not suggest that the progenitors of the neutron star and massive stars in the Carina Nebula, in particular η Car, 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.

Abstract Copyright:

Journal keyword(s): ISM: bubbles - stars: evolution - stars: formation - stars: neutron - supernova remnants - X-rays: stars

Simbad objects: 12

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2021.03.05-02:43:16

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