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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
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Generation of strong magnetic fields by r-modes in millisecond accreting neutron stars: Induced deformations and gravitational wave emission

Carmine Cuofano, +3 more
- 01 Aug 2012 - 
TL;DR: In this article, the magnetic damping term in the evolution equations of the r-modes was introduced and solved numerically in the Newtonian limit to follow the development and growth of the internal magnetic field.
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Some comments on the relativistic Thomas-Fermi model and the Vallarta-Rosen equation

Remo Ruffini, +1 more
- 02 Jul 1981 - 
TL;DR: In this paper, the basic differences between the screening of the nuclear charge due to a relativistic cloud of electrons in a neutral atom and the screening due to vacuum polarization effects induced by a superheavy ion are discussed.
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The discovery and study of the optical counterparts of the transient X-ray pulsars RX J0052.1-7319 and XTE J0111.2-7317 in the SMC

Stefano Covino, +6 more
- 01 Aug 2001 - 
TL;DR: In this article, the optical counterparts of the two transient X-ray pulsars, RX J0052.1-7319 and XTE J0111.2-7317.
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Short-term X-ray variability of the globular cluster source 4U 1820 - 30 (NGC 6624)

Luigi Stella, +2 more
- 15 Jul 1984 - 
TL;DR: In this paper, a large set of observations of the source 4U 1820 - 30 in the globular cluster NGC 6624 were used for improved identification of the temporal and spectral variability properties of X-ray sources.
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XMM-Newton and INTEGRAL view of the hard state of EXO 1745-248 during its 2015 outburst

M. Matranga, +13 more
- 01 Jul 2017 - 
TL;DR: In this article, a quasi-simultaneous XMM-Newton and INTEGRAL observations of the X-ray transient EXO 1745−248 located in the globular cluster Terzan 5, performed ten days after the beginning of the outburst (on 2015 March 16) of the source between March and June 2015.