1. A Close Encounter Of The Stellar Kind
... Astronomy Picture of the Day . A Close Encounter Of The Stellar Kind . << Yesterday . 7.07.2001 . Tomorrow >> . ... This future stellar encounter was discovered by researchers Joan Garcia-Sanchez and Robert Preston ( JPL ), and collaborators ...
2. APOD: 2001 July 7 - A Close Encounter Of The Stellar Kind
... 2001 July 7 . A Close Encounter Of The Stellar Kind . Credit: Digitized Sky Survey , SkyView . ... This future stellar encounter was discovered by researchers Joan Garcia-Sanchez and Robert Preston ( JPL ), and collaborators ...
4. http://hea-www.harvard.edu/~kim/pap/2013_GCLMXB_obs.pdf
... such as stellar age, GC mass, stellar encounter rate, and galacto-centric distance ... Figure 5. Histogram of GCs as a function of stellar encounter rate (). ... Another important parameter is the stellar encounter rate, , which takes both mass ...
5. Unexplained Brightening of Unusual Star | ESO
... In this dense stellar environment, close encounters between passing stars and ... The same close stellar encounters may also produce a diverse progeny of exotic ... primordial binaries in this cluster has been heavily modified by stellar encounters ...
6. Binary Radiopulsars with Black Holes
... The statistics obtained do not account for the BH binaries that could be formed in dense globular stellar clusters ? and then expelled from there due to possible stellar encounters (Kulkarni et al. ...
8. Sims Workshop Abstracts
... A further prediction is a high frequency of tight binary systems among massive stars due to tidal capture and the combination of tidal disruption followed by a star-disc encounter (failed stellar mergers). ...
9. http://xray.sai.msu.ru/~polar/sci_rev/0412.html
... astro-ph/0412030 Звездные взаимодействия как причина появления в Солнечной системе далеких объектов на эксцентричных орбитах (Stellar encounters as the origin of distant solar system objects in highly eccentric orbits) . ...
10. http://star.arm.ac.uk/preprints/2015/687.pdf
... for 60 magnetic lines inclination Time-dep endent diffusion calculations in stellar atmospheres present sp ecific difficulties not encountered in stellar interiors which have the advantage of b eing optically thick (see for instance Turcotte et al ...