Results 31 to 40 of about 53,953 (346)

Relations between Timing Features and Colors in the X-Ray Binary 4U 0614+09 [PDF]

open access: yes, 2000
We study the correlations between timing and X-ray spectral properties in the low-mass X-ray binary 4U 0614+09 using a large (265 ks) data set obtained with the Rossi X-Ray Timing Explorer.
S. van Straaten   +4 more
semanticscholar   +1 more source

Disc–jet coupling in an atoll-type neutron star X-ray binary: 4U 1728–34 (GX 354–0) [PDF]

open access: yes, 2003
We have analysed 12 simultaneous radio (Very Large Array) and X-ray (RXTE) observations of the atoll-type X-ray binary 4U 1728-34, performed in two blocks in 2000 and 2001.
S. Migliari   +6 more
semanticscholar   +1 more source

Physical parameters of the high-mass X-ray binary 4U1700-37 [PDF]

open access: yes, 2002
We present the results of a detailed non-LTE analysis of the ultraviolet and optical spectrum of the O6.5 Iaf + star HD 153919 - the mass donor in the high-mass X-ray binary 4U1700-37.
J. S. Clark   +11 more
semanticscholar   +1 more source

On X‐Ray Variability in Active Binary Stars

open access: yesThe Astrophysical Journal, 1999
We compare the count-rates of active binaries observed by Einstein and ROSAT. We find significant evidence for short-term variability (approx 0.32) and marginal evidence for a larger variability at longer timescales (approx 0.38). Modeling this excess as cyclic variability, we place an upper limit on the relative amplitude of the cyclic component ...
Kashyap, Vinay, Drake, Jeremy
openaire   +2 more sources

High-Mass X-Ray Binaries and OB Runaway Stars [PDF]

open access: yesInternational Astronomical Union Colloquium, 2004
AbstractHigh-mass X-ray binaries (HMXBs) represent an important phase in the evolution of massive binary systems and provide fundamental information on the properties of the OB-star primaries and their compact secondaries (neutron star, black hole). Recent observations indicate that the neutron stars in some of these systems (Vela X-1, 4U 1700-37) are ...
Kaper, L.   +2 more
openaire   +2 more sources

Search for intermittent X-ray pulsations from neutron stars in low-mass X-ray binaries [PDF]

open access: yesPublications of the Astronomical Society of Australia, 2021
AbstractWe present the results of our extensive binary orbital motion corrected pulsation search for 13 low-mass X-ray binaries. These selected sources exhibit burst oscillations in X-rays with frequencies ranging from 45 to 1 122 Hz and have a binary orbital period varying from 2.1 to 18.9 h.
Yunus Emre Bahar   +2 more
openaire   +4 more sources

SXP 1062, a young Be X-ray binary pulsar with long spin period - implications for the neutron star birth spin [PDF]

open access: yes, 2011
Context. The Small Magellanic Cloud (SMC) is ideally suited to investigating the recent star formation history from X-ray source population studies. It harbours a large number of Be/X-ray binaries (Be stars with an accreting neutron star as companion ...
F. Haberl   +4 more
semanticscholar   +1 more source

JET MODELS FOR NEUTRON STAR X-RAY BINARIES

open access: yesInternational Journal of Modern Physics: Conference Series, 2012
A variety of different models for jet formation have been developed over the years (mainly) for black hole systems and young stellar objects. Conclusive observational constraints which would favor one particular mechanism are difficult to obtain.
Migliari, S.   +3 more
openaire   +3 more sources

EVIDENCE FOR A CONSTANT INITIAL MASS FUNCTION IN EARLY-TYPE GALAXIES BASED ON THEIR X-RAY BINARY POPULATIONS, [PDF]

open access: yes, 2014
A number of recent studies have proposed that the stellar initial mass function (IMF) of early type galaxies varies systematically as a function of galaxy mass, with higher mass galaxies having bottom-heavy IMFs.
M. Peacock   +6 more
semanticscholar   +1 more source

Donor Stars in Black Hole X‐Ray Binaries [PDF]

open access: yesThe Astrophysical Journal, 1999
We study theoretically the formation of black-hole (BH) X-ray binaries. Consistency of the models with the observed relative numbers of systems with low-mass (<2 M_sun) and intermediate-mass (~2 M_sun - M_{BH}) donors leads to severe constraints on the evolutionary parameters of the progenitors.
openaire   +2 more sources

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