出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要:In the standard view describing the nature of long GRB emission, the duration of the centralengine activity has been usually considered to be much shorter that the afterglow emission variability time-scales. The discussion on the nature of X-ray flares and the recent studies on pre- and post-cursor emission observed in the gamma rays unveiled the possibility that the central-engine can be characterised by a much longer activity. In this work we discuss the signatures of late-time central-engine activity from a different perspective, i.e., in the temporal and spectral variability of the optical-NIR afterglow. We will discuss these signatures of the long-lasting central-engine activity unveiled thanks to the rich multicolour light curves obtained by the GROND instrument.