Search Results - "Hannikainen, Diana"
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Accretion states of the Galactic microquasar GRS 1758−258
Published in Monthly notices of the Royal Astronomical Society (21-07-2011)“…We present the results of a radio and X-ray study of the Galactic microquasar GRS 1758−258, using unpublished archival data and new observations. We focus in…”
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Accretion states of the Galactic microquasar GRS1758-258
Published in Monthly notices of the Royal Astronomical Society (21-07-2011)“…ABSTRACT We present the results of a radio and X-ray study of the Galactic microquasar GRS1758-258, using unpublished archival data and new observations. We…”
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Light curve morphology study of UW CrB – evidence for a 5 d superorbital period
Published in Monthly notices of the Royal Astronomical Society (01-04-2009)“…Since its discovery in 1990, UW CrB (also known as MS1603+2600) has remained a peculiar source without firm classification. Our current understanding is that…”
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Microquasars: A Galactic-Extragalactic Connection?
Published in Publications of the Astronomical Society of Australia (2002)“…Microquasars are Galactic X-ray binaries which show radio emission from relativistic outflows. Here we argue that the origins of radio emission from…”
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Similarities between Circular Polarization in Galactic Jet Sources and AGN
Published in Astrophysics and space science (01-01-2003)“…We compare the observational properties of the circular polarization in Galactic jet sources with that observed in AGN, and outline the constraints they place…”
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Spectral variability in Cygnus X-3
Published in Monthly notices of the Royal Astronomical Society (01-01-2009)“…We model the broad-band X-ray spectrum of Cyg X-3 in all states displayed by this source as observed by the Rossi X-ray Timing Explorer. From our models, we…”
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Light curve morphology study of UW CrB - evidence for a 5 d superorbital period
Published in Monthly notices of the Royal Astronomical Society (01-04-2009)Get full text
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Light curve morphology study of UW CrB - evidence for a 5 d superorbital period
Published in Monthly notices of the Royal Astronomical Society (2009)“…Since its discovery in 1990, UW CrB (also known as MS1603+2600) has remained a peculiar source without firm classification. Our current understanding is that…”
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Secrets behind the RXTE/ASM light curve of Cyg X-3
Published 13-05-2023“…A&A 674, A74 (2023) In wind-fed X-ray binaries, the radiatively driven wind of the primary star can be suppressed by the EUV irradiation of the compact…”
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XMM–Newton observations of UW CrB: detection of X-ray bursts and evidence for accretion disc evolution
Published in Monthly notices of the Royal Astronomical Society (01-01-2005)“…UW CrB (MS 1603+2600) is a peculiar short-period X-ray binary that exhibits extraordinary optical behaviour. The shape of the optical light curve of the system…”
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Pair annihilation and radio emission from galactic jet sources: the case of Nova Muscae
Published in Monthly notices of the Royal Astronomical Society (01-02-2002)Get full text
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Wind suppression by X-rays in Cygnus X-3
Published 06-04-2021“…A&A 649, A176 (2021) The radiatively driven wind of the primary star in wind-fed X-ray binaries can be suppressed by the X-ray irradiation of the compact…”
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XMM-Newton observations of UW CrB: detection of X-ray bursts and evidence for accretion disc evolution
Published in Monthly notices of the Royal Astronomical Society (01-01-2005)Get full text
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XTE J1550-564: a superluminal ejection during the September 1998 outburst
Published in Astrophysics and space science (01-01-2001)“…In 1998 September, the X-ray transient XTE J1550-564 underwent amajor outburst in soft and hard X-rays, followed by a radio flare. Australian Long Baseline…”
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Pair annihilation and radio emission from galactic jet sources: the case of Nova Muscae
Published in Monthly notices of the Royal Astronomical Society (11-02-2002)“…In the hard X-ray spectra of some X-ray binaries line features at around 500 keV are detected. We interpret these as arising from pair annihilation in…”
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Modeling the X-ray light curves of Cygnus X-3. Possible role of the jet
Published 16-12-2012“…Context: Physics behind the soft X-ray light curve asymmetries in Cygnus X-3, a well-known microquasar, was studied. AIMS: Observable effects of the jet close…”
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MOST radio observations of GX 339−4, GRS 1915+105 and GRO J1655−40
Published in New astronomy reviews (01-12-1998)“…We present results from the radio monitoring of the Galactic black hole candidates GX 339−4, GRS 1915+105 and GRO J1655−40 with the Molonglo Observatory…”
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RXTE and INTEGRAL observations of IGR J19140+0951
Published 07-01-2008“…AIP Conf.Proc.1010:266-268,2008 We have used the RXTE and INTEGRAL satellites simultaneously to observe the High Mass X-ray binary IGR J19140+0951. The spectra…”
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What Is a Parsec?
Published in Sky and telescope (01-12-2023)“…One of the most notoriously challenging aspects of astronomy is determining distances to faraway celestial objects. There's no way for us to take a cosmic tape…”
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