Search Results - "Cristofari, P"
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Particle acceleration in winds of star clusters
Published in Monthly notices of the Royal Astronomical Society (01-07-2021)“…ABSTRACT The origin of cosmic rays in our Galaxy remains a subject of active debate. While supernova remnant (SNR) shocks are often invoked as the sites of…”
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Constraining atmospheric parameters and surface magnetic fields with ZeeTurbo: an application to SPIRou spectra
Published in Monthly notices of the Royal Astronomical Society (13-04-2023)“…ABSTRACT We report first results on a method aimed at simultaneously characterizing atmospheric parameters and magnetic properties of M dwarfs from…”
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3
Estimating the atmospheric properties of 44 M dwarfs from SPIRou spectra
Published in Monthly notices of the Royal Astronomical Society (20-09-2022)“…ABSTRACT We describe advances on a method designed to derive accurate parameters of M dwarfs. Our analysis consists in comparing high-resolution infrared…”
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4
Estimating fundamental parameters of nearby M dwarfs from SPIRou spectra
Published in Monthly notices of the Royal Astronomical Society (10-02-2022)“…ABSTRACT We present the results of a study aiming at retrieving the fundamental parameters of M dwarfs from spectra secured with SPIRou, the near-infrared…”
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5
SPIRou monitoring of the protostar V347 Aur: binarity, magnetic fields, pulsed dynamo, and accretion
Published in Monthly notices of the Royal Astronomical Society (13-10-2024)“…ABSTRACT We present in this paper an analysis of near-infrared observations of the 0.3-${\rm M}_{\odot }$ protostar V347 Aurigae (V347 Aur) collected with the…”
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6
Gamma-rays from reaccelerated particles at supernova remnant shocks
Published in Monthly notices of the Royal Astronomical Society (11-10-2019)“…ABSTRACT Diffusive shock acceleration is considered as the main mechanism for particle energization in supernova remnants, as well as in other classes of…”
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7
The magnetic field and multiple planets of the young dwarf AU Mic
Published in Monthly notices of the Royal Astronomical Society (09-08-2023)“…ABSTRACT In this paper, we present an analysis of near-infrared spectropolarimetric and velocimetric data of the young M dwarf AU Mic, collected with SPIRou at…”
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8
Abundance matching for low-mass galaxies in the CDM and FDM models
Published in Monthly notices of the Royal Astronomical Society (01-02-2019)Get full text
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9
Monitoring the young planet host V1298 Tau with SPIRou: planetary system and evolving large-scale magnetic field
Published in Monthly notices of the Royal Astronomical Society (10-10-2023)“…ABSTRACT We report results of a spectropolarimetric monitoring of the young Sun-like star V1298 Tau based on data collected with the near-infrared…”
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10
Time-dependent high-energy gamma-ray signal from accelerated particles in core-collapse supernovae: the case of SN 1993J
Published in Monthly notices of the Royal Astronomical Society (2020)“…ABSTRACT Some core-collapse supernovae are likely to be efficient cosmic ray accelerators up to the PeV range, and therefore, to potentially play an important…”
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The classical T Tauri star CI Tau observed with SPIRou: magnetospheric accretion and planetary formation
Published in Monthly notices of the Royal Astronomical Society (05-04-2024)“…ABSTRACT We report new observations of the classical T Tauri star CI Tau with the SPIRou near-infrared spectropolarimeter and velocimeter at the…”
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12
Measuring small-scale magnetic fields of 44 M dwarfs from SPIRou spectra with ZeeTurbo
Published in Monthly notices of the Royal Astronomical Society (20-10-2023)“…ABSTRACT We present the results of an analysis aimed at probing the small-scale magnetic fields of M dwarfs observed with SPIRou, the nIR high-resolution…”
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13
Magnetic fields and rotation periods of M dwarfs from SPIRou spectra
Published in Monthly notices of the Royal Astronomical Society (01-10-2023)“…ABSTRACT We present near-infrared spectropolarimetric observations of a sample of 43 weakly to moderately active M dwarfs, carried with SPIRou at the…”
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14
Gamma-rays and neutrinos from RX J1713–3946 in a lepto–hadronic scenario
Published in Monthly notices of the Royal Astronomical Society (01-12-2021)“…ABSTRACT The gamma-ray emission of RX J1713–3946, despite being extensively studied in the GeV and TeV domains, remains poorly understood. This is mostly…”
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15
Acceleration of cosmic rays and gamma-ray emission from supernova remnants in the Galaxy
Published in Monthly notices of the Royal Astronomical Society (01-10-2013)“…Galactic cosmic rays are believed to be accelerated at supernova remnant shocks. Though very popular and robust, this conjecture still needs a conclusive…”
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16
On the search for Galactic supernova remnant PeVatrons with current TeV instruments
Published in Monthly notices of the Royal Astronomical Society (21-09-2018)“…The supernova remnant hypothesis for the origin of Galactic cosmic rays has passed several tests, but the firm identification of a supernova remnant PeVatron,…”
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The first days of Type II-P core collapse supernovae in the gamma-ray range
Published in Monthly notices of the Royal Astronomical Society (18-02-2022)“…ABSTRACT Type II-P supernovæ (SNe), the most common core-collapse SNe type, result from the explosions of red supergiant stars. Their detection in the radio…”
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SPIRou spectropolarimetry of the T Tauri star TW Hydrae: magnetic fields, accretion and planets
Published in Monthly notices of the Royal Astronomical Society (07-06-2024)“…In this paper we report near-infrared observations of the classical T Tauri star TW Hya with the SPIRou high-resolution spectropolarimeter and velocimeter at…”
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Active Cushing syndrome patients have increased ectopic fat deposition and bone marrow fat content compared to cured patients and healthy subjects: a pilot 1H-MRS study
Published in European journal of endocrinology (01-11-2018)“…Objective Glucocorticoid excess is one of the most important causes of bone disorders. Bone marrow fat (BMF) has been identified as a new mediator of bone…”
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The Hunt for Pevatrons: The Case of Supernova Remnants
Published in Universe (Basel) (01-09-2021)“…The search for Galactic pevatrons is now a well-identified key science project of all instruments operating in the very-high-energy domain. Indeed, in this…”
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