Nuclear activity and massive star formation in the low luminosity AGN NGC4303: Chandra X-ray observations

• Published in: arXiv.org 2003-04
• Main Authors: Jimenez-Bailon, Elena, Santos-Lleo, Maria, Jose Miguel Mas-Hesse, Guainazzi, Matteo, Colina, Luis, Cervino, Miguel, Gonzalez Delgado, Rosa M
• Format: Article
• Language: English
• Subjects: Active galactic nuclei; Astrometry; Binary stars; Emission; Galaxies; Linings; Luminosity; Massive stars; Soft x rays; Spatial resolution; Star & galaxy formation; Star clusters; Star formation; Stellar evolution; Supernova remnants; X ray sources; X-rays
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.0304465

We present evidence of the co-existence of either an AGN or an ultraluminous X-ray source (ULX), together with a young super stellar cluster in the 3 central parsecs of NGC4303. The galaxy contains a low luminosity AGN and hosts a number of starburst regions in a circumnuclear spiral, as well as in the nucleus itself. A high spatial resolution Chandra image of this source reveals that the soft X-ray emission traces the ultraviolet nuclear spiral down to a core, which is unresolved both in soft and hard X-rays. The astrometry of the X-ray core coincides with the UV core within the Chandra positioning accuracy. The total X-ray luminosity of the core, 1.5*10^{39} erg/s, is similar to that from some LINERs or from the weakest Seyferts detected so far. The soft X-rays in both the core and the extended structure surrounding it can be well reproduced by evolutionary synthesis models (which include the emission expected from single stars, the hot diffuse gas, supernova remnants and binary systems), consistent with the properties of the young stellar clusters identified in the UV. The hard X-ray tail detected in the core spectrum, however, most likely requires the presence of an additional source. This additional source could either be a weak active nucleus black hole or an ultraluminous X-ray object. The implications of these results are discussed.