scispace - formally typeset
L

Luigi Stella

Researcher at INAF

Publications -  779
Citations -  38625

Luigi Stella is an academic researcher from INAF. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 92, co-authored 771 publications receiving 36266 citations. Previous affiliations of Luigi Stella include European Space Agency & Bosch.

Papers
More filters
Journal ArticleDOI

Swift observations of SAX J1808.4-3658: monitoring the return to quiescence

Sergio Campana, +2 more
- 28 Jul 2008 - 
TL;DR: In this article, the transition from outburst to quiescence of a millisecond pulsar SAX J1808.4-3658 has been investigated in detail using the Swift observing flexibility.
Journal Article

The changing soft X-ray light curve of the AM Her system MR Serpentis (PG 1550+191)

Lorella Angelini, +2 more
- 01 Aug 1990 - 
TL;DR: In this article, the first soft X-ray light curves of the AM Her system MR Ser were obtained within a 4-month interval in 1984, all obtained within the EXOSA T low-energy telescope, and one observation was made in which MR Ser was the target.
Journal ArticleDOI

The supergiant fast X-ray transients XTE J1739-302 and IGR J08408-4503 in quiescence with XMM-Newton

Enrico Bozzo, +8 more
- 12 Apr 2010 - 
TL;DR: In this article, the authors used three XMM-Newton observations of the two supergiant fast X-ray transient prototypes XTEJ1739-302 and IGR J08408-4503 in quiescence.
Proceedings ArticleDOI

Proposal to do fast x-ray timing with XEUS

Ruediger Staubert, +8 more
- 10 Mar 2003 - 
TL;DR: In this paper, a proposal for an added capability of fast timing to the European x-ray astronomy mission XEUS is described, which is used to probe strong gravity fields around collapsed objects and to constrain the equation of state of dense matter in neutron stars.
Journal ArticleDOI

BeppoSAX observations of the black hole candidates LMC X-1 and LMC X-3

Aldo Treves, +8 more
- 01 Apr 1999 - 
TL;DR: In this paper, the authors describe BeppoSAX observations of the black hole candidates LMC X--1 and LMCX--3 performed in Oct. 1997, and find no indication of emission or absorption features whatsoever.