Search Results - "Gelfand, Joseph"
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Emission-line velocity, metallicity, and extinction maps of the Large Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (18-03-2024)“…ABSTRACT We measure the properties of optical emission lines in multiple locations across the Large Magellanic Cloud (LMC) using the Australian National…”
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2
Dependence of the Radio Emission on the Eddington Ratio of Radio-quiet Quasars
Published in The Astrophysical journal (01-09-2022)“…Abstract Roughly 10% of quasars are “radio-loud,” producing copious radio emission in large jets. The origin of the low-level radio emission seen from the…”
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The radio emission in radio-quiet quasars: the VLBA perspective
Published in Monthly notices of the Royal Astronomical Society (09-08-2023)“…ABSTRACT The origin of the radio emission in radio-quiet quasars (RQQ) is not established yet. We present new VLBA observations at 1.6 and 4.9 GHz of 10 RQQ (9…”
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4
Discovery of GeV Gamma-Ray Emission from Pulsar Wind Nebula Kes 75 and PSR J1846–0258
Published in The Astrophysical journal (01-01-2023)“…Abstract We report the detection of gamma-ray emission from pulsar wind nebula (PWN) Kes 75 and PSR J1846−0258. Through modeling the spectral energy…”
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Broadband X-Ray Spectroscopy of the Pulsar Wind Nebula in HESS J1640-465
Published in The Astrophysical journal (01-03-2023)“…Abstract We present updated measurements of the X-ray properties of the pulsar wind nebula associated with the TeV γ -ray source HESS J1640-465 derived from…”
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A Dynamical Model for the Evolution of a Pulsar Wind Nebula Inside a Nonradiative Supernova Remnant
Published in The Astrophysical journal (01-10-2009)“…A pulsar wind nebula (PWN) inside a supernova remnant provides a unique insight into the properties of the central neutron star, the relativistic wind powered…”
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A Massive Shell of Supernova-formed Dust in SNR G54.1+0.3
Published in The Astrophysical journal (10-02-2017)“…While theoretical models of dust condensation predict that most refractory elements produced in core-collapse supernovae (SNe) efficiently condense into dust,…”
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The Nonstandard Properties of a “Standard” PWN: Unveiling the Mysteries of PWN G21.5–0.9 Using Its IR and X-Ray Emission
Published in The Astrophysical journal (01-11-2020)“…Abstract The evolution of a pulsar wind nebula (PWN) depends on properties of the progenitor star, supernova, and surrounding environment. As some of these…”
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9
Suppressing star formation in quiescent galaxies with supermassive black hole winds
Published in Nature (London) (26-05-2016)“…In order for quiescent galaxies to maintain their low-to-non-existent star formation, there must be a mechanism to remove or heat gas that would otherwise cool…”
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10
Windy or Not: Radio Parsec-scale Evidence for a Broad-line Region Wind in Radio-quiet Quasars
Published in The Astrophysical journal (01-11-2024)“…Abstract Does a broad-line region (BLR) wind in radio-quiet (RQ) active galactic nuclei (AGN) extend to parsec scales and produce radio emission? We explore…”
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Hard X-Ray Observation and Multiwavelength Study of the PeVatron Candidate Pulsar Wind Nebula “Dragonfly”
Published in The Astrophysical journal (01-09-2023)“…Abstract We studied the PeVatron nature of the pulsar wind nebula (PWN) G75.2+0.1 (“Dragonfly”) as part of our NuSTAR observational campaign of energetic PWNe…”
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12
Probing the History of the Galaxy Assembly of the Counterrotating Disk Galaxy PGC 66551
Published in The Astrophysical journal (01-02-2024)“…Abstract Stellar counterrotation in disk galaxies directly relates to the complex phenomenon of the disk mass assembly believed to be driven by external…”
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The Impact of Low-luminosity AGNs on Their Host Galaxies: A Radio and Optical Investigation of the Kiloparsec-scale Outflow in MaNGA 1-166919
Published in The Astrophysical journal (01-08-2021)“…Abstract One way an active galactic nucleus (AGN) influences the evolution of their host galaxy is by generating a large-scale (kiloparsec-scale) outflow. The…”
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THE PROPERTIES OF THE PROGENITOR SUPERNOVA, PULSAR WIND, AND NEUTRON STAR INSIDE PWN G54.1+0.3
Published in The Astrophysical journal (01-07-2015)“…ABSTRACT The evolution of a pulsar wind nebula (PWN) inside a supernova remnant (SNR) is sensitive to the properties of the central neutron star, pulsar wind,…”
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The origin of UV/optical emission in the black hole low-mass X-ray binary Swift J1753.5–0127
Published in Monthly notices of the Royal Astronomical Society (01-07-2022)“…ABSTRACT The emission from the accreting black holes (BHs) in low-mass X-ray binaries (LMXBs) covers a broad energy band from radio to X-rays. Studying the…”
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Relation between spectral changes and the presence of the lower kHz QPO in the neutron star low-mass X-ray binary 4U 1636−53
Published in Monthly notices of the Royal Astronomical Society (11-03-2017)“…We fitted the 3-180 keV spectrum of all the observations of the neutron star low-mass X-ray binary 4U 1636-53 taken with the Rossi X-ray Timing Explorer using…”
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Fermi-LAT Gamma-Ray Emission Discovered from the Composite Supernova Remnant B0453-685 in the Large Magellanic Cloud
Published in The Astrophysical journal (01-03-2023)“…Abstract We report the second extragalactic pulsar wind nebula (PWN) to be detected in the megaelectronvolt–gigaelectronvolt band by the Fermi-LAT, located…”
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JWST Constraints on the UV Luminosity Density at Cosmic Dawn: Implications for 21 cm Cosmology
Published in Astrophysical journal. Letters (01-11-2023)“…Abstract An unprecedented array of new observational capabilities are starting to yield key constraints on models of the epoch of first light in the Universe…”
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Parkes Radio and NuSTAR X-Ray Observations of the Composite Supernova Remnant B0453–685 in the Large Magellanic Cloud
Published in The Astrophysical journal (01-11-2024)“…Abstract Gamma-ray emission is observed coincident in position to the evolved, composite supernova remnant (SNR) B0453–685. Prior multiwavelength…”
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Investigating Galactic Supernova Remnant Candidates Using LOFAR
Published in The Astrophysical journal (20-06-2018)“…We investigate six supernova remnant (SNR) candidates-G51.21+0.11, G52.37-0.70, G53.07+0.49, G53.41+0.03, G53.84-0.75, and the possible shell around…”
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