Name: L* meeting
Start: 2023-01-30T09:00:00+00:00
End: 2023-02-03T12:00:00+00:00
Location: No location set

3D thermal evolution of magnetars with the new finite volume code MATINS

A puzzling 2-hour X-ray periodicity in the 1.5-hour orbital period black widow PSR J1311-3430

A systematic view on cyclotron lie sources with NuSTAR

Accreting Millisecond X-ray Pulsars: observational properties

Beyond X-ray Timing

CHORD: a new attack to the FRB science

Concluding remarks

Conclusions & Open Discussion

CubeSats and Distributed Astronomy: from the HERMES fleet to the flight of the ALBATROS, surfing the waves of quantum space-time

Da EXOSAT a Swift: piu' di 35 anni di collaborazione con Luigi

Does a quasi-universal structured jet model successfully the short GRB population?

Evolution and multiwavelength emission properties of ULX binary systems accreting above Eddington

FRBs under the lens: a unified model

Gamma Ray Burst cosmic evolution

High Resolution and Broad Band Spectra of NS LMXB: A review

High-energy emission and disk/jet connection in Galactic black-hole binaries

IXPE results on accreting black holes

Luigi's contribution

Ma alla fine chi paga la bolletta?

Matter ejections behind the highs and lows of a transitional pulsar

Multimessenger Gamma-Ray Bursts

OUVERTURE PER UN AMENO SIMPOSIO: Dove si narra di nane ciccione e di altre bizzarre creature che vagano per la Via Lattea solitarie o accoppiate

Propeller: from V0332 to IGRJ18245

Relativistic effects in massive binary millisecond pulsars found by MeerKAT

Relatività e righe del ferro relativistiche

Riusciranno i nostri eroi...?

The Relativistic Precession Model from birth to maturity - part 1

The Relativistic Precession Model from birth to maturity - part 2

The spin distribution of magnetars from birth to elder times

Timing analysis of the 2022 outburst of SAX J1808.4-3658: hints of an orbital shrinking

Transitional millisecond pulsars: a tale of two powers

Transitional white dwarfs

Two shades of variability: a new pulsar in the Large Magellanic Cloud and a QPO in M51 ULX-7

Ultime novità dalla doppia pulsar a 20 anni dalla sua scoperta

What can we learn from ULX pulsar (spectral) timing?

Working with Luigi on X-ray binary systems

X-ray Polarimetry of Accreting Neutron Stars and Magnetars

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L* meeting