CERN Accelerating science

CERN Document Server 73 elementer funnet  1 - 10nesteslutt  gå til element: Søket tok 0.73 sekunder. 
1.
Measuring The Thickness Of The Magellanic Cloud Cepheid Population : Implications For Microlensing / Graff, D ; Bauer, F ; Afonso, C ; Albert, J N ; Andersen, J ; Ansari, R ; Aubourg, E ; Bareyre, P ; Beaulieu, J P ; Bouquet, A et al.
PCC-98-26.
- 1998.
IN2P3 Publications database
2.
Not enough stellar mass objects to fill the Galactic halo? / Milshtein, A I
The Universe contains a lot more than meets the eye. Sophisticated experiments search diligently for this invisible dark matter. [...]
2000 - Published in : CERN Cour.: 40 (2000) , no. 4, pp. 13-15 External link: CERN Courier server
3.
$a_{1}(1260)\pi$ dominance in the process $e^+ e^- \to 4\pi$ at energies 1.05 - 1.38 GeV / Akhmetshin, R R ; Anashkin, E V ; Arpagaus, M ; Aulchenko, V M ; Banzarov, V S ; Barkov, L M ; Bashtovoy, N S ; Bondar, A E ; Bondarev, D V ; Bragin, A V et al.
BUDKER-INP-98-83.
- 1998. - 33 p.
Access to fulltext document - Access to fulltext document
4.
On the role of the $a_{1}(1260)$ meson in $\tau \to 4 \pi \nu_{\tau}$ decay / Bondar, A E ; Eidelman, S I ; Milshtein, A I ; Root, N I
It is shown that a simple model successfully describing experimental data on the process e/sup +/e/sup -/ to 4 pi can also qualitatively account for the data of CLEOII and ALEPH obtained recently in the decay tau to 4 pi nu /sub tau /. The model is based on the assumption of the a/sub 1/(1260) pi and omega pi dominance as intermediate states. [...]
1999 - Published in : Phys. Lett. B 466 (1999) 403-7
5.
EROS 2 proper motion survey : a field brown dwarf and an L dwarf companion to LHS 102 / EROS Collaboration
We report the discovery of two L dwarfs (the new spectral class defined for dwarfs cooler than the M type) in a two-epoch CCD proper motion survey of 413 square degrees, complemented by infrared photometry from DENIS. One of them has a strong lithium line and is therefore a brown dwarf. [...]
astro-ph/9905162.- 1999 - Published in : Astron. Astrophys. 351 (1999) L5 Access to fulltext document: 9905162.fig.3a - PS.GZ; 9905162.fig.3b - PS.GZ; 9905162 - PDF; External link: astro-ph/9905162 PDF
6.
Observation of Microlensing towards the Galactic Spiral Arms : EROS II 2 year survey / EROS Collaboration
We present the analysis of the light curves of 8.5 million stars observed during two seasons by EROS (Experience de Recherche d'Objets Sombres), in the galactic plane away from the bulge. Three stars have been found that exhibit luminosity variations compatible with gravitational microlensing effects due to unseen objects. [...]
astro-ph/9903209; CERN-OPEN-99-069; LAL-99-12.- Geneva : CERN, 1999 - 11 p. - Published in : Astron. Astrophys. 351 (1999) 87 External link: Fulltext
7.
The two EROS 4Kx8K CCD mosaic cameras / Bauer, F ; Adrianzyk, G ; Afonso, C ; Albert, J N ; Andersen, J ; Ansari, R ; Aubourg, E ; Aune, S ; Baranne, A ; Bareyre, P et al.
1997 - Published in : Nucl. Instrum. Methods Phys. Res., A 387 (1997) 286 Access to fulltext document: TIF PDF; - CERN library copies
8.
The $Q^{2}$ dependence of the structure function ratio $F^{Sn}_{2}/F^{C}_{2}$ and the difference $R^{Sn}-R^{C}$ in deep inelastic muon scattering / New Muon Collaboration
1996 - Published in : Nucl. Phys. B 481 (1996) 23-39
9.
The $A$ dependence of the nuclear structure function ratios / New Muon Collaboration
1996 - Published in : Nucl. Phys. B 481 (1996) 3-22
10.
Azimuthal asymmetry in processes of nonlinear QED for linearly polarized photon / Baier, V N ; Milshtein, A I
BUDKER-INP-94-83.
- 1994. - 13 p.
Access to fulltext document - Access to fulltext document - CERN library copies

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