stochastic star formation and a (nearly) uniform stellar
... galaxy SFR. The IGIMF implementation follows the minimal-1 and minimal-2 formulations (Pflamm-Altenburg et al. 2007), with a Kroupa (2001) IMF and a CMF with β = 2, minimum mass of 20 M and maximum mass derived from the SFR averaged over 107 yr. In both the Kroupa fc = 1 and the IGIMF model, the IM ...
... galaxy SFR. The IGIMF implementation follows the minimal-1 and minimal-2 formulations (Pflamm-Altenburg et al. 2007), with a Kroupa (2001) IMF and a CMF with β = 2, minimum mass of 20 M and maximum mass derived from the SFR averaged over 107 yr. In both the Kroupa fc = 1 and the IGIMF model, the IM ...
![arXiv:1210.2471v1 [astro-ph.EP] 9 Oct 2012 Exoplanet Detection](http://s1.studyres.com/store/data/015975823_1-e4b4b3613f38bbff39746aa9bc12073b-300x300.png)
Study properties of dwarf galaxies in and around the nearby Lynx
... Voids are delineated by luminous (L > L*) massive objects and populated by dwarfs. The galaxy densities and other parameters vary significantly from one void to another. One expects that not only galaxy interactions occur in voids much less frequently, but also DM halo and galaxy formation from dens ...
... Voids are delineated by luminous (L > L*) massive objects and populated by dwarfs. The galaxy densities and other parameters vary significantly from one void to another. One expects that not only galaxy interactions occur in voids much less frequently, but also DM halo and galaxy formation from dens ...
SPY — The ESO Supernovae Type Ia Progenitor Survey
... DO white dwarfs). We routinely measure RVs with an accuracy of about 2 km/s, therefore running only a very small risk of missing a merger precursor, which have orbital velocities of 150 km/s or higher. The large programme was finished at the end of last semester. A total of 1014 stars were observed ...
... DO white dwarfs). We routinely measure RVs with an accuracy of about 2 km/s, therefore running only a very small risk of missing a merger precursor, which have orbital velocities of 150 km/s or higher. The large programme was finished at the end of last semester. A total of 1014 stars were observed ...
A Tale of Two Physics
... This paper offers an alternative explanation for Dark Matter, Dark Energy, and their unexpected causal linkage by creating an alternative version using a leg of Laplace's and Le Sage’s Shadow theory. A geometric proof is derived that explains the origins of Dark Energy and Dark Matter, predicting bo ...
... This paper offers an alternative explanation for Dark Matter, Dark Energy, and their unexpected causal linkage by creating an alternative version using a leg of Laplace's and Le Sage’s Shadow theory. A geometric proof is derived that explains the origins of Dark Energy and Dark Matter, predicting bo ...
Genesis of the Heaviest Elements in the Milky Way Galaxy
... course still less than that of the Sun, but the relative abundance of this -process element to Fe in many of these stars can be much larger than the solar ratio. This star-to-star scatter diminishes with increasing metallicity tending toward younger stars. While there could be several possible exp ...
... course still less than that of the Sun, but the relative abundance of this -process element to Fe in many of these stars can be much larger than the solar ratio. This star-to-star scatter diminishes with increasing metallicity tending toward younger stars. While there could be several possible exp ...
Meade Introduction: 7" Mak, 8", 10" and 12"
... such as the Orion Nebula are visible in such wide extension that the nebulosity may fill the field of view. This listing only hints at the breadth of galactic and extragalactic objects visible through the eyepiece of a Meade 8", 10", or 12" SCT model: it is a rare observer who might in a lifetime vi ...
... such as the Orion Nebula are visible in such wide extension that the nebulosity may fill the field of view. This listing only hints at the breadth of galactic and extragalactic objects visible through the eyepiece of a Meade 8", 10", or 12" SCT model: it is a rare observer who might in a lifetime vi ...
Confirmation of Hostless Type Ia Supernovae Using Hubble Space
... truly belonged to the intracluster stellar population we used the HST ACS to obtain deep images at their locations. We waited until >3 years after peak brightness to obtain these images to avoid contamination from the SN itself (this is discussed in Section 3.5). To either rule out or classify a fai ...
... truly belonged to the intracluster stellar population we used the HST ACS to obtain deep images at their locations. We waited until >3 years after peak brightness to obtain these images to avoid contamination from the SN itself (this is discussed in Section 3.5). To either rule out or classify a fai ...
STAR CLUSTERS M. Ramella e G. Iafrate INAF – Astronomical
... and sizes, but it is important to remember that these differences may be only apparent since they depend on the different distances from us of the objects. This is a common situation in astronomy: we measure apparent properties (in this case the angular size), but in order to understand the nature o ...
... and sizes, but it is important to remember that these differences may be only apparent since they depend on the different distances from us of the objects. This is a common situation in astronomy: we measure apparent properties (in this case the angular size), but in order to understand the nature o ...
Leica Polarization brochure - Earth-2
... The screen illumination level possible with these two projection methods is usually great enough so that the classroom need only partially be darkened. A reduction in stray light, however, enhances the effects. The less “uninvited” light, the clearer your image will be. Placing the projector close t ...
... The screen illumination level possible with these two projection methods is usually great enough so that the classroom need only partially be darkened. A reduction in stray light, however, enhances the effects. The less “uninvited” light, the clearer your image will be. Placing the projector close t ...
The paper on the Hubble constant published in 2010
... Abstract: It is shown that the Hubble constant can be derived from the standard luminosity function of galaxies as well as from a new luminosity function as deduced from the mass-luminosity relationship for galaxies. An analytical expression for the Hubble constant can be found from the maximum numb ...
... Abstract: It is shown that the Hubble constant can be derived from the standard luminosity function of galaxies as well as from a new luminosity function as deduced from the mass-luminosity relationship for galaxies. An analytical expression for the Hubble constant can be found from the maximum numb ...
SimulationDatabases
... Data sets are often very large, often far away (makes them even larger!) To analyse remote datasets, one needs to be able to bring the analysis to the data. “Standard” approach using flat files and C/IDL/etc code sub-optimal To analyse very large datasets we also need advanced methods of dat ...
... Data sets are often very large, often far away (makes them even larger!) To analyse remote datasets, one needs to be able to bring the analysis to the data. “Standard” approach using flat files and C/IDL/etc code sub-optimal To analyse very large datasets we also need advanced methods of dat ...
1 Brief History of the Discovery of Phenomena Concerning Light
... primary spherical wave, a secondary ellipsoidal wave. It was in the course of this investigation that Huygens made the fundamental discovery of polarization in 1690: each of the two rays arising from refraction by calcit may be extinguished by passing it through a second crystal of the same material ...
... primary spherical wave, a secondary ellipsoidal wave. It was in the course of this investigation that Huygens made the fundamental discovery of polarization in 1690: each of the two rays arising from refraction by calcit may be extinguished by passing it through a second crystal of the same material ...