GaAs(331)A面InAs自组织纳米结构形貌演化

采用分子束外延方法在CaAs(331)A高指数衬底上制备自对齐InAs纳米线(QWRs)或者三维(3D)岛状结构.InAs纳米线(QWRs)选择性生长在CaAs层的台阶边缘.通过原子力显微镜(AfM)仔细研究了InAs纳米微结构的表面形貌,发现不同的生长条件,包括:衬底温度、生长速率、和InAs层厚度等,对InAa表面形貌有很大的影响.如,低温更容易导致线状纳米微结构的形成,而高温更利于3D岛状结构形成.表面形貌的转变归结于表面能同应变能之间的竞争.

Response to comment on “The response of vegetation on the Andean flank in western Amazonia to Pleistocene climate change” – M.L. Cárdenas et al., Science 331, 1055 (25 February 2011)”.

Puyasena et al. question our interpretation of climate-driven vegetation change on the Andean flank in western Amazonia during the middle Pleistocene and suggest that the use of Podocarpus spp. as a proxy of past climate change should be reassessed. We defend our assertion that vegetation change at the Erazo study site was predominantly driven by climate change due to concomitant changes recorded by multiple taxa in the fossil record.

Concerning CP violation in 331 models

We consider the implementation of CP violation in the context of 331 models. In particular we treat a model where only three scaler triplets are needed in order to give all fermions a mass while keeping neutrino massless. In this case all CP violation is provided by the scalar sector.

Efeitos de Z' nos modelos left-right, B-L e 331

Pós-graduação em Física - IFT

The young stellar cluster [DBS2003] 157 associated with the H ii region GAL 331.31-00.34

We report a study of the stellar content of the near-infrared (NIR) cluster [DBS2003] 157 embedded in the extended H ii region GAL 331.31-00.34, which is associated with the IRAS source 16085-5138. JHK photometry was carried out in order to identify potential ionizing candidates, and the follow-up NIR spectroscopy allowed the spectral classification of some sources, including two O-type stars. A combination of NIR photometry and spectroscopy data was used to obtain the distance of these two stars, with the method of spectroscopic parallax: IRS 298 (O6 V, 3.35 +/- 0.61 kpc) and IRS 339 (O9 V, 3.24 +/- 0.56 kpc). Adopting the average distance of 3.29 +/- 0.58 kpc and comparing the Lyman continuum luminosity of these stars with that required to account for the radio continuum flux of the H ii region, we conclude that these two stars are the ionizing sources of GAL 331.31-00.34. Young stellar objects (YSOs) were searched by using our NIR photometry and mid-infrared (MIR) data from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) survey. The analysis of NIR and MIR colourcolour diagrams resulted in 47 YSO candidates. The GLIMPSE counterpart of IRAS 16085-5138, which presents IRAS colour indices compatible with an ultracompact H ii region, has been identified. The analysis of its spectral energy distribution between 2 and m revealed that this source shows a spectral index a= 3.6 between 2 and m, which is typical of a YSO immersed in a protostellar envelope. Lower limits to the bolometric luminosity and the mass of the embedded protostar have been estimated as L= 7.7 x 10(3) L? and M= 10 M?, respectively, which correspond to a B0B1 V zero-age main sequence star.

Na 50 Nachlass Arthur Schopenhauer - 'Schopenhauer-Archiv', 331 - Mitteilung an Professor Hugo von Meltzl über weitere potentielle Ansatzpunkte für die Schopenhauer-Forschung

u.a.: Arthur Schopenhauer; Ferdinand Laban; Dr. Meinong; David Hume;

Ms.Ff.F.Stoltze 3. 331 - Brief von Friedrich Stoltze an Jacob Daltroff

Friedrich Stoltze II: Rose vom Grab