Search Results - "FILIPOVIC, M. D"
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The spectral energy distribution of powerful starburst galaxies – I. Modelling the radio continuum
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract We have acquired radio-continuum data between 70 MHz and 48 GHz for a sample of 19 southern starburst galaxies at moderate redshifts…”
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The physical parameters of the microquasar S26 in the Sculptor Group galaxy NGC 7793
Published in Monthly notices of the Royal Astronomical Society (01-12-2012)“…NGC 7793−S26 is an extended source (350 pc × 185 pc) previously studied in the radio, optical and X-ray domains. It has been identified as a microquasar which…”
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Early-stage young stellar objects in the Small Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (01-02-2013)“…We present new observations of 34 young stellar object (YSO) candidates in the Small Magellanic Cloud (SMC). The photometric selection required sources to be…”
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Multifrequency study of the Large Magellanic Cloud supernova remnant J0529−6653 near pulsar B0529-66
Published in Monthly notices of the Royal Astronomical Society (01-03-2012)“…We report the Australia Telescope Compact Array (ATCA) and ROSAT detection of supernova remnant (SNR) J0529−6653 in the Large Magellanic Cloud (LMC) which is…”
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An evolutionary sequence of young radio galaxies
Published in Astronomische Nachrichten (01-02-2016)“…We have observed the faintest sample of Gigahertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) sources to date, using the Australia Telescope Compact…”
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Radio-continuum detections of Galactic Planetary Nebulae - I. MASH PNe detected in large-scale radio surveys
Published in Monthly notices of the Royal Astronomical Society (21-03-2011)“…We present an updated and newly compiled radio-continuum data base for Macquarie/AAO/Strasbourg Hα (MASH) planetary nebulae (PNe) detected in the extant…”
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Multiwavelength study of a new Galactic SNR G332.5−5.6
Published in Monthly notices of the Royal Astronomical Society (11-10-2007)“…We present compelling evidence for confirmation of a Galactic supernova remnant (SNR) candidate, G332.5−5.6, based initially on identification of new,…”
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Radio planetary nebulae in the Magellanic Clouds
Published in Monthly notices of the Royal Astronomical Society (21-10-2009)“…We report the extragalactic radio-continuum detection of 15 planetary nebulae (PNe) in the Magellanic Clouds (MCs) from recent Australia Telescope Compact…”
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Daily variations of indoor air-ion and radon concentrations
Published in Applied radiation and isotopes (01-11-2009)“…Air-ions and radon are two atmospheric trace constituents which have two opposite effects on human health: the ions are beneficial, and radon gas is…”
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An ATCA radio-continuum study of the Small Magellanic Cloud – V. Long-slit optical spectroscopy of supernova remnants and confirmation of a new candidate supernova remnant
Published in Monthly notices of the Royal Astronomical Society (21-04-2007)“…We present optical long-slit spectra and estimated line ratios for 11 of the 16 known radio supernova remnants (SNRs) in the Small Magellanic Cloud (SMC) using…”
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An ATCA radio-continuum study of the Small Magellanic Cloud — III. Supernova remnants and their environments
Published in Monthly notices of the Royal Astronomical Society (01-11-2005)“…A total of 717 sources from the Australia Telescope Compact Array (ATCA) catalogue of the Small Magellanic Cloud (SMC) have been classified in Paper II (of…”
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Swings between rotation and accretion power in a binary millisecond pulsar
Published in Nature (London) (26-09-2013)“…A neutron star with a low mass companion star was observed at different times as a millisecond pulsar powered either by the rotation of its magnetic field or…”
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ALMA CO Observations of the Mixed-morphology Supernova Remnant W49B: Efficient Production of Recombining Plasma and Hadronic Gamma Rays via Shock–Cloud Interactions
Published in The Astrophysical journal (01-10-2021)“…Abstract We carried out new CO( J = 2–1) observations toward the mixed-morphology supernova remnant (SNR) W49B with the Atacama Large Millimeter/submillimeter…”
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An ATCA radio-continuum study of the Small Magellanic Cloud - IV. A multifrequency analysis of the N 66 region
Published in Monthly notices of the Royal Astronomical Society (21-04-2006)“…Traditional identification of supernova remnants (SNRs) include the use of radio spectral index, optical spectral studies (including strong [S ii], [N ii], [O…”
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ON THE EXPANSION RATE, AGE, AND DISTANCE OF THE SUPERNOVA REMNANT G266.2–1.2 (Vela Jr.)
Published in The Astrophysical journal (10-01-2015)“…An analysis of Chandra ACIS data for two relatively bright and narrow portions of the northwestern rim of G266.2-1.2 (a.k.a. RX J0852.0-4622 or Vela Jr.)…”
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An Expanding Shell of Neutral Hydrogen Associated with SN 1006: Hints for the Single-degenerate Origin and Faint Hadronic Gamma-Rays
Published in The Astrophysical journal (01-07-2022)“…Abstract We report new H i observations of the Type Ia supernova remnant (SNR) SN 1006 using the Australia Telescope Compact Array with an angular resolution…”
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Discovery of a Wind-blown Bubble Associated with the Supernova Remnant G346.6-0.2: A Hint for the Origin of Recombining Plasma
Published in The Astrophysical journal (01-12-2021)“…Abstract We report on CO and H i studies of the mixed-morphology supernova remnant (SNR) G346.6−0.2. We find a wind-blown bubble along the radio continuum…”
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Determination of Planetary Nebulae angular diameters from radio continuum spectral energy distribution modelling
Published in Monthly notices of the Royal Astronomical Society (01-05-2021)“…ABSTRACT Powerful new, high-resolution, high-sensitivity, multifrequency, wide-field radio surveys such as the Australian Square Kilometre Array Pathfinder…”
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ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons
Published in The Astrophysical journal (01-10-2020)“…N132D is the brightest gamma-ray supernova remnant (SNR) in the Large Magellanic Cloud (LMC). We carried out 12CO(J = 1-0, 3-2) observations toward the SNR…”
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XMMU J050722.1−684758: discovery of a new Be X-ray binary pulsar likely associated with the supernova remnant MCSNR J0507−6847
Published in Monthly notices of the Royal Astronomical Society (17-04-2021)“…ABSTRACT We report the discovery of a new high-mass X-ray binary pulsar, XMMU J050722.1−684758, possibly associated with the supernova remnant (SNR) MCSNR…”
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