Search Results - "De martino, D"
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Constraining the evolution of cataclysmic variables via the masses and accretion rates of their underlying white dwarfs
Published in Monthly notices of the Royal Astronomical Society (01-03-2022)“…ABSTRACT We report on the masses (MWD), effective temperatures ($\rm{T_\mathrm{eff}}$), and secular mean accretion rates ($\langle \dot{M} \rangle$) of 43…”
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The peculiar bursting nature of CP Pup
Published in Monthly notices of the Royal Astronomical Society (01-03-2024)“…ABSTRACT The classical nova CP Puppis has been observed to have particularly puzzling and peculiar properties. In particular, this classical nova displays…”
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Pulsating in Unison at Optical and X-Ray Energies: Simultaneous High Time Resolution Observations of the Transitional Millisecond Pulsar PSR J1023+0038
Published in The Astrophysical journal (10-09-2019)“…PSR J1023+0038 is the first millisecond pulsar discovered to pulsate in the visible band; such a detection took place when the pulsar was surrounded by an…”
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4
Discovery of persistent quasi-periodic oscillations in accreting white dwarfs: a new link to X-ray binaries
Published in Monthly notices of the Royal Astronomical Society (17-10-2024)“…ABSTRACT Almost all accreting black hole and neutron star (NS) X-ray binary systems (XRBs) exhibit prominent brightness variations on a few characteristic…”
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Multiwavelength observations of the transitional millisecond pulsar binary XSS J12270−4859
Published in Monthly notices of the Royal Astronomical Society (01-12-2015)“…We present an analysis of X-ray, ultraviolet and optical/near-IR photometric data of the transitional millisecond pulsar binary XSS J12270...4859, obtained at…”
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6
Long-period Radio Pulsars: Population Study in the Neutron Star and White Dwarf Rotating Dipole Scenarios
Published in The Astrophysical journal (01-02-2024)“…Abstract The nature of two recently discovered radio emitters with unusually long periods of 18 minutes (GLEAM-X J1627–52) and 21 minutes (GPM J1839–10) is…”
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Enhanced optical activity 12 d before X-ray activity, and a 4 d X-ray delay during outburst rise, in a low-mass X-ray binary
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT X-ray transients, such as accreting neutron stars, periodically undergo outbursts, thought to be caused by a thermal-viscous instability in the…”
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Search for multiwavelength emission from the binary millisecond pulsar PSR J1836-2354A in the globular cluster M22
Published in Monthly notices of the Royal Astronomical Society (01-07-2019)“…ABSTRACT We present a multiband search for X-ray, optical, and γ-ray emission of the radio binary millisecond pulsar J1836-2354A, hosted in the globular…”
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9
Evidence for mass accretion driven by spiral shocks onto the white dwarf in SDSS J123813.73–033933.0
Published in Monthly notices of the Royal Astronomical Society (11-02-2019)Get full text
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10
Genome-scale estimate of the metabolic turnover of E. coli from the energy balance analysis
Published in Physical biology (29-01-2016)“…In this article the notion of metabolic turnover is revisited in the light of recent results of out-of-equilibrium thermodynamics. By means of Monte Carlo…”
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11
SDSS unveils a population of intrinsically faint cataclysmic variables at the minimum orbital period
Published in Monthly notices of the Royal Astronomical Society (21-08-2009)“…We discuss the properties of 137 cataclysmic variables (CVs) which are included in the Sloan Digital Sky Survey (SDSS) spectroscopic data base, and for which…”
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Swift J201424.9+152930: discovery of a new deeply eclipsing binary with 491-s and 3.4-h modulations
Published in Monthly notices of the Royal Astronomical Society (21-06-2015)“…We report on the discovery of a new X-ray pulsator, Swift J201424.9+152930 (Sw J2014). Owing to its X-ray modulation at 491 s, it was discovered in a…”
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13
The true nature of Swift J0746.3-1608: a possible Intermediate Polar showing accretion state changes
Published in Monthly notices of the Royal Astronomical Society (21-03-2019)Get full text
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14
IGR J14257−6117, a magnetic accreting white dwarf with a very strong strong X-ray orbital modulation
Published in Monthly notices of the Royal Astronomical Society (21-07-2018)Get full text
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15
Burst-induced spin variations in the accreting magnetic white dwarf PBC J0801.2–4625
Published in Monthly notices of the Royal Astronomical Society (06-05-2024)“…ABSTRACT PBC J0801.2–4625 is an intermediate polar with a primary spin frequency of 66.08 d−1 and an unknown orbital period. The long-term All Sky Automated…”
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Gaia white dwarfs within 40 pc – I. Spectroscopic observations of new candidates
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…ABSTRACT We present a spectroscopic survey of 230 white dwarf candidates within 40 pc of the Sun from the William Herschel Telescope and Gran Telescopio…”
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Triggering micronovae through magnetically confined accretion flows in accreting white dwarfs
Published in Monthly notices of the Royal Astronomical Society (01-07-2022)“…ABSTRACT Rapid bursts at optical wavelengths have been reported for several accreting white dwarfs. In these bursts, the optical luminosity can increase by up…”
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2PBC J0658.0–1746: a hard X-ray eclipsing polar in the orbital period gap
Published in Monthly notices of the Royal Astronomical Society (11-10-2019)“…Abstract The hard X-ray source 2PBC J0658.0–1746 was proposed as an eclipsing magnetic cataclysmic variable of the polar type, based on optical follow-ups. We…”
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Effective temperatures of cataclysmic-variable white dwarfs as a probe of their evolution
Published in Monthly notices of the Royal Astronomical Society (21-04-2017)“…Abstract We present HST spectroscopy for 45 cataclysmic variables (CVs), observed with HST/COS and HST/STIS. For 36 CVs, the white dwarf is recognisable…”
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Gaia white dwarfs within 40 pc – III. Spectroscopic observations of new candidates in the Southern hemisphere
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…Abstract We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the Southern hemisphere. Observations…”
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