Search Results - "Palacio, S del"
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New Insights into the H ii Region G18.88-0.49: Hub-Filament System and Accreting Filaments
Published in The Astrophysical journal (01-11-2020)“…We present an analysis of multiwavelength observations of an area of 0 27 × 0 27 around the Galactic H ii region G18.88−0.49, which is powered by an O-type…”
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2
The High-Energy Emission from HD 93129A Near Periastron
Published in Monthly notices of the Royal Astronomical Society (01-06-2020)“…We conducted an observational campaign towards one of the most massive and luminous colliding wind binaries in the Galaxy, HD 93129A, close to its periastron…”
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3
Probing the Physical Conditions and Star Formation Processes in the Galactic H II Region S305
Published in The Astrophysical journal (01-08-2020)“…We present multiscale and multiwavelength observations of the Galactic H ii region S305, which is excited by massive O8.5V and O9.5V stars. Infrared images…”
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PSR J0437-4715: The Argentine Institute of Radioastronomy 2019-2020 Observational Campaign
Published in The Astrophysical journal (01-02-2021)“…We present the first-year data set of high-cadence, long-duration observations of the bright millisecond pulsar J0437−4715 obtained in the Argentine Institute…”
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5
A shared accretion instability for black holes and neutron stars
Published in Nature (London) (02-03-2023)“…Accretion disks around compact objects are expected to enter an unstable phase at high luminosity 1 . One instability may occur when the radiation pressure…”
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6
Bow shocks, nova shells, disc winds and tilted discs: the nova-like V341 Ara has it all
Published in Monthly notices of the Royal Astronomical Society (01-02-2021)“…ABSTRACT V341 Ara was recently recognized as one of the closest (d ≃ 150 pc) and brightest (V ≃ 10) nova-like cataclysmic variables. This unique system is…”
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7
Evidence for non-thermal X-ray emission from the double WR colliding-wind binary Apep
Published 16-02-2023“…A&A 672, A109 (2023) Context: Massive colliding-wind binaries (CWBs) can be non-thermal sources. The emission produced in their wind-collision region (WCR)…”
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The non-thermal emission from the colliding-wind binary Apep
Published 17-12-2021“…Publ. Astron. Soc. Aust. 39 (2022) e004 The recently discovered massive binary system Apep is the most powerful synchrotron emitter among the known Galactic…”
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Exploring the physics behind the non-thermal emission from star-forming galaxies detected in gamma rays
Published 23-09-2021“…A&A 657, A49 (2022) Star-forming galaxies (SFGs) emit non-thermal radiation from radio to gamma-rays. We aim to investigate the main mechanisms of global CR…”
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10
Non-thermal emission in hyper-velocity and semi-relativistic stars
Published 23-03-2022“…A&A 661, A102 (2022) Context. There is a population of runaway stars that move at extremely high speeds with respect to their surroundings. The fast motion and…”
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Joint ALMA/X-ray monitoring of the radio-quiet type 1 AGN IC 4329A
Published 28-03-2024“…A&A 690, A232 (2024) The origin of a compact millimeter (mm, 100-250 GHz) emission in radio-quiet active galactic nuclei (RQ AGN) remains debated. Recent…”
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12
New insights in the HII region G18.88-0.49: hub-filament system and accreting filaments
Published 11-09-2020“…We present an analysis of multi-wavelength observations of an area of 0.27 deg x 0.27 deg around the Galactic HII region G18.88-0.49, which is powered by an…”
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13
A shared accretion instability for black holes and neutron stars
Published 28-02-2023“…Accretion disks around compact objects are expected to enter an unstable phase at high luminosity. One instability may occur when the radiation pressure…”
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14
The gamma-ray / infrared luminosity correlation of star-forming galaxies
Published 15-07-2020“…A&A 641, A147 (2020) Context. Near a dozen star-forming galaxies have been detected in gamma-rays by the Fermi observatory in the last decade. A remarkable…”
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15
Probing the physical conditions and star formation processes in the Galactic HII region S305
Published 05-06-2020“…We present multi-scale and multi-wavelength observations of the Galactic HII region S305, which is excited by massive O8.5V and O9.5V stars. Infrared images…”
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16
Radio observations of evaporating objects in the Cygnus OB2 region
Published 17-04-2019“…We present observations of the Cygnus OB2 region obtained with the Giant Metrewave Radio Telescope (GMRT) at the frequencies of 325 MHz and 610 MHz. In this…”
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17
PSR J0437-4715: The Argentine Institute of Radioastronomy 2019-2020 Observational Campaign
Published 28-01-2021“…The Argentine Institute of Radio astronomy (IAR) is equipped with two single-dish 30-m radio antennas capable of performing daily observations of pulsars and…”
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18
A persistent ultraviolet outflow from an accreting neutron star binary transient
Published 02-03-2022“…All disc-accreting astrophysical objects produce powerful outflows. In binaries containing neutron stars (NS) or black holes, accretion often takes place…”
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19
A persistent ultraviolet outflow from an accreting neutron star binary transient
Published in Nature (London) (03-03-2022)“…All disc-accreting astrophysical objects produce powerful disc winds. In compact binaries containing neutron stars or black holes, accretion often takes place…”
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20
Multi-zone non-thermal radiative model for stellar bowshocks
Published 01-07-2018“…A&A 617, A13 (2018) Context: Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non-thermal radio emission has been…”
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