Search Results - "La Palombara, N"
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1
Spectral properties of the soft excess pulsar RX J0059.2–7138 during its 2013 outburst
Published in Monthly notices of the Royal Astronomical Society (01-06-2015)“…We report on an X-ray observation of the Be X-ray binary pulsar RX J0059.2–7138, performed by XMM–Newton in 2014 March. The 19 ks long observation was carried…”
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2
XTE J1906+090: a persistent low-luminosity Be X-ray binary
Published in Monthly notices of the Royal Astronomical Society (23-05-2023)“…ABSTRACT We present new results from INTEGRAL and Swift observations of the hitherto poorly studied and unidentified X-ray source XTE J1906+090. A bright hard…”
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3
Multiwavelength investigation of the candidate Galactic PeVatron MGRO J1908+06
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT The candidate PeVatron MGRO J1908+06, which shows a hard spectrum beyond 100 TeV, is one of the most peculiar γ-ray sources in the Galactic plane. Its…”
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4
New X-ray observations of the hot subdwarf binary HD 49798/RX J0648.0–4418
Published in Monthly notices of the Royal Astronomical Society (22-04-2021)“…ABSTRACT HD 49798/RX J0648.0–4418 is the only confirmed X-ray binary in which the mass donor is a hot subdwarf star of O spectral type and, most likely, it…”
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5
Spectral analysis of SMC X-2 during its 2015 outburst
Published in Monthly notices of the Royal Astronomical Society. Letters (01-05-2016)“…We report on the results of XMM–Newton and Swift observations of SMC X-2 during its last outburst in 2015 October, the first one since 2000. The source reached…”
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6
X-Ray Observation of the Roche-lobe-filling White Dwarf plus Hot Subdwarf System ZTF J213056.71+442046.5
Published in The Astrophysical journal (01-05-2022)“…Abstract ZTF J213056.71+442046.5 is the prototype of a small class of recently discovered compact binaries composed of a white dwarf and a hot subdwarf that…”
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7
Ultramassive, Fast-Spinning White Dwarf in a Peculiar Binary System
Published in Science (American Association for the Advancement of Science) (04-09-2009)“…White dwarfs typically have masses in a narrow range centered at about 0.6 solar mass (M[middle dot in circle]). Only a few ultramassive white dwarfs (mass >…”
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8
X-ray emission from hot subdwarfs with compact companions
Published in EPJ Web of conferences (01-01-2013)“…We review the X-ray observations of hot subdwarf stars. While no X-ray emission has been detected yet from binaries containing B-type subdwarfs, interesting…”
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9
Spectral analysis of IGR J01572−7259 during its 2016 outburst
Published in Monthly notices of the Royal Astronomical Society (21-03-2018)“…Abstract We report on the results of the XMM–Newton observation of IGR J01572−7259 during its most recent outburst in 2016 May, the first since 2008. The…”
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10
Constraints on the winds of hot subdwarf stars from X-ray observations of two sdB binaries with compact companions: CD −30° 11223 and PG 1232–136
Published in Monthly notices of the Royal Astronomical Society (01-07-2014)“…Little observational data are available on the weak stellar winds of hot subdwarf stars of B spectral type (sdB). Close binary systems composed of an sdB star…”
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X-RAY AND OPTICAL OBSERVATIONS OF THE UNIQUE BINARY SYSTEM HD 49798/RX J0648.0-4418
Published in The Astrophysical journal (20-08-2011)“…We report the results of XMM-Newton observations of HD 49798/RX J0648.0-4418, the only known X-ray binary consisting of a hot sub-dwarf and a white dwarf. The…”
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12
Multiwavelength observations of the two unidentified EGRET sources 3EG J0616-3310 and 3EG J1249-8330
Published in Astrophysics and space science (01-06-2007)“…Issue Title: The Multi-Messenger Approach to High-Energy Gamma-Ray Sources: Third Workshop on the Nature of Unidentified High-Energy Sources We report on the…”
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13
The Cherenkov optics qualification facilities at INAF-OAB laboratories
Published in Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment (01-02-2020)“…In the last decade the Osservatorio Astronomico di Brera of the Italain Institute for Astrophysics, INAF, got deeply involved in Cherenkov optics manufacturing…”
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14
Detection of the Crab Nebula with the 9.7 m prototype Schwarzschild-Couder telescope
Published in Astroparticle physics (01-03-2021)“…The Schwarzschild-Couder Telescope (SCT) is a telescope concept proposed for the Cherenkov Telescope Array. It employs a dual-mirror optical design to remove…”
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15
The optical/UV filters for the EPIC experiment
Published in IEEE transactions on nuclear science (01-06-1998)“…EPIC, the European Photon Imaging Cameras is an experiment based on cooled CCDs on board the ESA X-ray Multi Mirrors satellite due to be launched in 1999…”
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16
Scientific prospects for a mini-array of ASTRI telescopes: A γ-ray TeV data challenge
Published in Journal of high energy astrophysics (01-06-2020)“…ASTRI is a project aiming at the realization of a γ-ray imaging Cherenkov telescope that observes the sky in the TeV band. Recently, the development of a…”
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17
XTE J1906+090: a persistent low luminosity Be X-ray Binary
Published 11-05-2023“…We present new results from INTEGRAL and Swift observations of the hitherto poorly studied and unidentified X-ray source XTE J1906+090. A bright hard X-ray…”
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18
News on the X-ray emission from hot subdwarf stars
Published 01-12-2017“…In latest years, the high sensitivity of the instruments on-board the XMM-Newton and Chandra satellites allowed us to explore the properties of the X-ray…”
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Follow-up observations of X-ray emitting hot subdwarf stars: the compact He-poor sdO star Feige 34
Published 09-03-2021“…A&A 626, A29 (2019) We report on results obtained with the XMM-Newton observation of Feige 34 carried out in April 2018. This is the first spectroscopic X-ray…”
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20
On the nature of the 2.4 hr-period eclipsing cataclysmic variable W2 in 47 Tuc
Published 04-07-2024“…A&A 689, A176 (2024) W2 (CXOGlb J002415.8-720436) is a cataclysmic variable (CV) in the Galactic globular cluster 47 Tucanae. Its modulation was discovered…”
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