close-binaries
A study of early type close binaries
... The dot-dashed line represents the terminal-age main sequence of Bressan et ale 1981 including convective overshooting and mass loss... The Mass-Luminosity diagram for those objects plot[r] ...
431
Post common envelope binaries from SDSS II : identification of 9 close binaries with VLT/FORS2
... all close compact binary sys- tems ranging from X-ray binaries to double white dwarf binaries or cataclysmic variables, to name a few, have formed through CE ...
11
Simulations of stripped core-collapse supernovae in close binaries
... a close binary system, and study the effects of the explosion on the companion star as well as the effect of the presence of the companion on the supernova ...
19
PG1258+593 and its common proper motion magnetic white dwarf counterpart
... and close) WD plus M-dwarf binaries (Silvestri et ...M-dwarf binaries, ...of close binaries generate strong magnetic fields in the core of the WD ...
8
Detached cataclysmic variables are crossing the orbital period gap
... detached close binaries consisting of a WD and an M4–M6 secondary ...such binaries with known periods below 10 h to 52 ...envelope binaries (PCEBs) alone and that the existence of dCVs is ...
12
14 new eclipsing white dwarf plus main-sequence binaries from the SDSS and Catalina surveys
... Two of the close binaries listed in Table 3 have slightly odd light curves, which are shown in Figure 7. In both cases there is a sinusoidal variation on half the orbital period, similar to el- lipsoidal ...
13
WRAP_MNRAS-2016-Bours-3873-87.pdf
... in close binaries to measure apparent and/or real variations in their orbital ...67 close binaries, both detached and semi-detached and with M-dwarfs, K-dwarfs, brown dwarfs or white dwarfs ...
16
Post common envelope binaries from SDSS VIII, Evidence for disrupted magnetic braking
... and close binaries that suffered from dynamically unsta- ble mass transfer, ...WDMS binaries, and to determine their bi- nary ...WDMS binaries, identify 205 strong PCEB candi- dates and ...
5
Long-term eclipse timing of white dwarf binaries: an observational hint of a magnetic mechanism at work
... NN Ser is a white dwarf + M-dwarf binary with an or- bital period of 3.1 h, showing not only eclipses but also a large reflection effect. This system has been studied ex- tensively, both photometrically and ...
17
Testing the universality of star formation - II. Comparing separation distributions of nearby star-forming regions and the field
... There is a possible weak trend of decreasing MF with increasing density in all separation ranges, including, unexpectedly, the 19– 100 au unprocessed range. In the 62–620 au range, the separation distributions of all our ...
11
Faint galactic X ray binaries
... X–ray binaries have been ...X–ray binaries as well as the supergiant fast X–ray transients, lower resolution X–ray images together with especially 2MASS often provide a fair assessment of the source ...
9
Fuzzing binaries with Lévy flight swarms
... Our aim (as motivated at the beginning of this section) is to adapt the diffusion parameters in such a way that the algorithm automatically focuses its search (by decreasing diffusivity [r] ...
10
An investigation of contact and non contact binary systems
... Plot of mass against radius for the data on late-type contact and near-contact binaries shown in Table 9.1, together with Popper's 1980 data for main sequence detached binaries.. The dat[r] ...
367
Particle acceleration in binaries
... object, which is a Wolf-Rayet star. But Cygnus X-3 shows a short orbital period of 4.8 hours, typical of low mass binaries. It has been inferred from the modulation of both X-ray (Fig. 6) and infrared emissions. ...
6
D2T3 - Stefano Zanero - Behaviour-Based Methods for Automated Scalable Malware Analysis.pdf
... genotype model match always corresponds to presence of code implementing the behavior. Also no false positives against dataset of ~2000 benign binaries binaries in system32 on a win[r] ...
41
System parameters of X Ray binaries
... Schematic view of an XRB, including the Roche lobe filling companion star, the mass transfer stream, and the accretion disc around the compact object, shown in both spatial coordinates X[r] ...
187
Spitzer microlens measurement of a massive remnant in a well separated binary
... All known stellar-mass black holes ( BHs ) are in close binary systems. Presumably this is a selection effect induced by the fact that these BHs have been detected via X-ray emission generated by accretion from a ...
12
14 65 04 7801 IAS 2 0 pdf
... QR303 -A- Single-use license, binaries, key source modules, documentation, support services media: D, E, T QR303 -C- Single-use license, binaries, key source modules, documentation, no s[r] ...
5
Wobbling ancient binaries - here be planets?
... In the case of the remaining two systems, NN Ser and UZ For, our dynamical simulations reveal that the candidate companions would move on orbits that are stable on long timescales. As a result, the existence of ...
14
Kink and Feminism – Breaking the Binaries
... Challenging the Euro centrism of much of psychoanalysis, Ghent writes, “In the West surrender has meant "defeat." In the East it has meant transcendence, liberation. In the West "ego", as used in the ...
8