Browsing by Subject "ISM: jets and outflows"

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  • Fast launch speeds in radio flares, from a new determination of the intrinsic motions of SS 433's jet bolides 
    Jeffrey R.; Blundell K.; Trushkin S.; Mioduszewski A. (2016)
    © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.We present newhigh-resolution, multi-epoch, Very Long BaselineArray (VLBA) radio images of the Galactic microquasar SS ...
  • LOFAR 150-MHz observations of SS 433 and W50 
    Trushkin S.; Stewart A.; Anderson G.; Staley T.; Blundell K.; Pietka M.; Markoff S.; Rowlinson A.; Swinbank J.; van der Horst A.; Bell M.; Breton R.; Carbone D.; Corbel S.; Eislöffel J.; Falcke H.; Grießmeier J.; Hessels J.; Kondratiev V.; Law C.; Molenaar G.; Serylak M.; Stappers B.; van Leeuwen J.; Wijers R.; Wijnands R.; Wise M.; Zarka P. (2018)
    © 2017 The Author(s). We present Low-Frequency Array (LOFAR) high-band data over the frequency range 115-189 MHz for the X-ray binary SS 433, obtained in an observing campaign from 2013 February to 2014 May. Our results ...
  • On the Apparent Absence of Wolf-Rayet+Neutron Star Systems: The Curious Case of WR124 
    Toalá J.; Oskinova L.; Hamann W.; Ignace R.; Sander A.; Shenar T.; Todt H.; Chu Y.; Guerrero M.; Hainich R.; Torrejón J. (2018)
    © 2018. The American Astronomical Society. All rights reserved.. Among the different types of massive stars in advanced evolutionary stages is the enigmatic WN8h type. There are only a few Wolf-Rayet (WR) stars with this ...
  • Strong low-frequency radio flaring from Cygnus X-3 observed with LOFAR 
    Broderick J.W.; Russell T.D.; Fender R.P.; Trushkin S.A.; Green D.A.; Chauhan J.; Nizhelskij N.A.; Tsybulev P.G.; Bursov N.N.; Shevchenko A.V.; Pooley G.G.; Williams D.R.A.; Bright J.S.; Rowlinson A.; Corbel S. (2021)
    We present Low-Frequency Array (LOFAR) 143.5-MHz radio observations of flaring activity during 2019 May from the X-ray binary Cygnus X-3. Similar to radio observations of previous outbursts from Cygnus X-3, we find that ...

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