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pro vyhledávání: '"Ercan, N."'
Publikováno v:
In Revue Française d'Allergologie February 2023 63(1)
Akademický článek
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Publikováno v:
In Revue Française d'Allergologie October 2019 59(6):411-414
Publikováno v:
Astrophys.Space Sci.324:17-22,2009
Optical CCD imaging with H$\alpha$ and [SII] filters and spectroscopic observations of the galactic supernova remnant G85.9-0.6 have been performed for the first time. The CCD image data are taken with the 1.5m Russian-Turkish Telescope (RTT150) at T
Externí odkaz:
http://arxiv.org/abs/0909.2959
Autor:
Del Popolo, A., Ercan, N.
In this paper, I revisit the constraints obtained by several authors (Reichart et al. 1999; Eke et al. 1998; Henry 2000) on the estimated values of $\Omega_{\rm m}$, $n$ and $\sigma_8$ in the light of recent theoretical developments: 1) new theoretic
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508663
Publikováno v:
Astron.Astrophys.432:771,2005
In this paper, we discuss improvements of the Suto et al. (2000) model, in the light of recent theoretical developments (new theoretical mass functions, a more accurate mass-temperature relation and an improved bias model) to predict the clustering p
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508592
Autor:
Del Popolo, A., Ercan, N.
In this paper, I revisit the constraints obtained by several authors (Reichart et al. 1999; Eke et al. 1998; Henry 2000) on the estimated values of Omegam, n and sigma_8 in the light of recent theoretical developments: 1) new theoretical mass functio
Externí odkaz:
http://arxiv.org/abs/astro-ph/0404382
Publikováno v:
Int.J.Mod.Phys.D12:1399-1414,2003
In the current paper, we further improved the model for the migration of planets introduced in Del Popolo et al. (2001) and extended to time-dependent planetesimal accretion disks in Del Popolo and Eksi (2002). In the current study, the assumption of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0308021
Publikováno v:
Mon.Not.Roy.Astron.Soc. 339 (2003) 556
In this paper, we further develop the model for the migration of planets introduced in Del Popolo, Gambera and Ercan, and extended to time-dependent planetesimal accretion disks in Del Popolo and Eksi. More precisely, the assumption of Del Popolo and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0303654
Publikováno v:
Astron.J. 122 (2001) 487-495
We study the non-linear evolution of a dust ellipsoid,embedded in a Friedmann flat background universe, in order to determine the evolution of the density of the ellipsoid as the perturbation to it related detaches from general expansion and begins t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0108080