The hypersoft state of Cygnus X-3: A key to jet quenching in X-ray binaries?© ESO 2018. Context. Cygnus X-3 is
a unique microquasar in the Galaxy hosting
a Wolf
Photoionization Emission Models for the Cyg X-3 X-Ray SpectrumKallman T.,
McCollough M.,
Koljonen K.,
Liedahl D.,
Miller J.,
Paerels F.,
Pooley G.,
Sako M.,
Schulz N.,
Trushkin S.,
Corrales L. for the narrow feature seen near the Si
K edge. We identify the features of
a wind in the profiles of the strong
Strong low-frequency radio flaring from Cygnus X-3 observed with LOFARBroderick 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. X-3, we find that this source was significantly variable at low frequencies, reaching
a maximum flux
Breast cancer risk genes - Association analysis in more than 113,000 womenDorling, L.,
Carvalho, S.,
Allen, J.,
González-Neira, A.,
Luccarini, C.,
Wahlström, C.,
Pooley, K.A.,
Parsons, M.T.,
Fortuno, C.,
Wang, Q.,
Bolla, M.K.,
Dennis, J.,
Bermisheva, M.,
Khusnutdinova, E.,
Prokofyeva, D.,
other additional authors , and reliable subtype-specific risk estimates are lacking. METHODS We used
a panel of 34 putative susceptibility
The giant flares of the microquasar Cygnus X-3: X-rays states and jets, consisting of
a Wolf-Rayet star and probably
a black hole. The first flare occurred on 13 September 2016
Optical Counterparts of ULXs and Their Host Environments in NGC 4490/4485 NGC 4490/4485. Using archival Hubble Space Telescope (HST) imaging data, we identified
a single
Developing the structure of the personality's ecological cultureThe article is devoted to
a detailed analysis of the personality's ecological cultureand