The equations of medieval cosmology     

Roberto Buonanno  Claudia Quercellini 《New Astronomy》2009,14(3):347-348

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Stellar clusters in the nuclear regions of AGN with the Advanced Camera for Surveys     

Víctor M. Muñoz Marín  Rosa M. González Delgado  Henrique R. Schmitt  Roberto Cid Fernandes  Enrique Pérez 《Astrophysics and Space Science》2009,324(2-4):253-258

We explore the role of star clusters in the nuclear regions of galaxies through their connection with active galactic nuclei (AGN). Nuclear star clusters (NCs) are conspicuous in the centers of most nearby galaxies, all along the Hubble sequence. These clusters are probably the faint-end distribution of the central supermassive black holes (SMBHs) in massive bulges. On the other hand, star formation is known to be ongoing in the majority of Seyfert nuclei and in many low-luminosity active galactic nuclei (LLAGN). We study two samples of AGN galaxies (75 Seyferts and 26 LLAGN) in the near-ultraviolet with the Hubble Space Telescope’s Advanced Camera for Surveys. We aim to better understand the connection between the growing of the SMBH and the build-up of the bulge, and we also intend to make statistical progress and determine the properties of the population of NCs coexisting with growing SMBHs.  相似文献   

Kinematics of gas and stars in circumnuclear star-forming regions of early-type spirals     

Guillermo F. Hägele  Ángeles I. Díaz  Mónica V. Cardaci  Elena Terlevich  Roberto Terlevich 《Astrophysics and Space Science》2009,324(2-4):341-342

We present high-resolution (R～20,000) spectra in the blue and the far red of circumnuclear star-forming regions (CNSFRs) in three early-type spirals (NGC3351, NGC2903 and NGC3310), which have allowed the study of the kinematics of the stars and the ionized gas in these structures and, for the first time, the derivation of their dynamical masses for the first two. In some cases, these regions, about 100 to 150 pc in size, are composed of several individual star clusters with sizes between 1.5 and 4.9 pc, estimated from Hubble Space Telescope images. The stellar dispersions have been obtained from the Calcium triplet (CaT) lines at λ λ 8494, 8542, 8662 Å, while the gas velocity dispersions have been measured by means of Gaussian fits to the Hβ and [Oiii]λ 5007 Å lines in the high-dispersion spectra. Values of the stellar velocity dispersions are between 30 and 68 km?s^?1. We apply the virial theorem to estimate dynamical masses of the clusters, assuming that systems are gravitationally bounded and spherically symmetric, and using previously measured sizes. The measured values of the stellar velocity dispersions yield dynamical masses of the order of 10⁷ to 10⁸ M_⊙ for the entire CNSFRs. Stellar and gas velocity dispersions are found to differ by about 20 to 30 km?s^?1, with the Hβ emission lines being narrower than both the stellar lines and the [Oiii]λ 5007 Å lines. The douby-ionized oxygen, on the other hand, exhibits velocity dispersions comparable to those of the stars or, in some cases, even larger. We have found indications of the presence of two different kinematical components in the ionized gas of the regions. We have mapped the velocity field in the central kpc of the spiral galaxies NGC3351 and NGC2903. For the first object, the radial velocity curve shows deviations from circular motions for the ionized hydrogen consistent with its infall towards the central regions of the galaxy, at a velocity of about 25 km?s^?1. For NGC3310, we present preliminary results for the velocity dispersions for one of the two observed slit position angles, two CNSFRs and the nucleus.  相似文献   

A Moon-borne electromagnetic calorimeter     

Roberto Battiston  Maria Teresa Brunetti  Franco Cervelli  Cristiano Fidani  Mauro Menichelli 《Astrophysics and Space Science》2009,323(4):357-366

We discuss an electromagnetic sampling calorimeter for the detection of very high energy gamma-rays on the Moon, which is based on the use of scintillating cylinders and plates imbedded in the lunar soil. The use of lunar soil as a calorimeter radiator reduces the weight of the material to be transported to the Moon and minimises environmental impact. Plastic scintillator bars inserted into the regolith about 1.5 m are the active elements of this instrument: at the surface, each bar is terminated by a plastic scintillator plate to veto high energy charge particles. The readout system for the scintillator bars and plates are based on recently developed single photon solid state detectors (Silicon Photomultiplier, SiPM), extremely compact, sturdy and sensitive devices suited for detecting small light pulses in a space experiment. The performance of a regolith-scintillator calorimeter is evaluated and the relevant parameters are optimised using a GEANT4 simulation.  相似文献   

The spatial distribution of X-ray selected AGN in the Chandra deep fields: a theoretical perspective     

Federico Marulli  Silvia Bonoli  Enzo Branchini  Roberto Gilli  Lauro Moscardini  Volker Springel 《Monthly notices of the Royal Astronomical Society》2009,396(3):1404-1414

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On the derivation of dynamical masses of the stellar clusters in the circumnuclear region of NGC 2903     

Guillermo F. Hägele  Ángeles I. Díaz  Mónica V. Cardaci †  Elena Terlevich ‡  Roberto Terlevich ‡ 《Monthly notices of the Royal Astronomical Society》2009,396(4):2295-2312

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Visible continuum emission and gravity waves     

A. Molina 《Planetary and Space Science》1983,31(3):331-337

Observed oscillations in the visible continuum emission (5000 Å) are studied considering the usual visible emission mechanism, NO + O (both two-body and three-body paths). Characteristic parameters of internal gravity waves are obtained using Hines' linear theory. Values of the kinetic energy density ?, and temperature variations Δθ, due to gravity waves are calculated. The results (? ~ 10⁶cm²s^?2, Δθ = 4–9K) are in agreement with those obtained by means of different techniques reported in the literature. A similar analysis of the simultaneous green-line emission data is made and a comparison is drawn between the results obtained for both emissions. An expression relating relative brightness of continuum emission and relative perturbations of atmospheric density is proposed.  相似文献   

Bayesian calibrated significance levels applied to the spectral tilt and hemispherical asymmetry     

Christopher Gordon  Roberto Trotta 《Monthly notices of the Royal Astronomical Society》2007,382(4):1859-1863

Bayesian model selection provides a formal method of determining the level of support for new parameters in a model. However, if there is not a specific enough underlying physical motivation for the new parameters it can be hard to assign them meaningful priors, an essential ingredient of Bayesian model selection. Here we look at methods maximizing the prior so as to work out what is the maximum support the data could give for the new parameters. If the maximum support is not high enough then one can confidently conclude that the new parameters are unnecessary without needing to worry that some other prior may make them significant. We discuss a computationally efficient means of doing this which involves mapping p-values on to upper bounds of the Bayes factor (or odds) for the new parameters. A p-value of 0.05 (1.96σ) corresponds to odds less than or equal to 5:2, which is below the 'weak' support at best threshold. A p-value of 0.0003 (3.6σ) corresponds to odds of less than or equal to 150:1, which is the 'strong' support at best threshold. Applying this method we find that the odds on the scalar spectral index being different from one are 49:1 at best. We also find that the odds that there is primordial hemispherical asymmetry in the cosmic microwave background are 9:1 at best.  相似文献   

Effects of physical phenomena on the distribution of nutrients and phytoplankton productivity in a coastal lagoon     

Roberto Millan-Nuñez  Saul Alvarez-Borrego  David M. Nelson 《Estuarine, Coastal and Shelf Science》1982,15(3):317-335

Sea level, salinity, temperature, nitrate, nitrite, phosphate, silicate, chlorophylls a, b and c and their phaeophytins, phytoplankton abundance and phytoplankton productivity time series were generated for the mouth and three interior locations of Bahia San Quintin, Baja California, Mexico, for 10 days during summer of 1979. The samples were taken once every 2 h. This was done to describe space and time variability of these ecological properties and to elucidate the main factors that cause this variability. Upwelling events bring nutrient reach waters near the bay mouth and tidal currents propagate those waters throughout the bay. Nutrient remineralization at the sediments and the effect of turbulence induced by tidal currents and winds increase nutrient concentrations in the interiors of the bay. In comparison with available information on nutrients limited growth of planktonic algae, nutrients seemed not to be limiting to phytoplankton growth during the sampling period. Phytoplankton cell abundances at the extremes of the lagoon are an order of magnitude lower than at the mouth due to greater turbidity. Chlorophyll concentrations at the extremes are about one-third of those of the mouth. Primary productivity decreases from the mouth to the interiors in the same manner as chlorophyll does. There is not a significant difference in cell size between phytoplankton at the bay mouth and those at the extremes of the bay. Primary productivity in the bay is comparable to the productivity maxima of other upwelling areas. There is no clear permanent dominance of diatoms over dinoflagellates, or vice versa, at any location in the bay. The alternation of upwelling and non-upwelling played an important role, together with that of the spring-neap tide cycle, in producing low frequency (< 0.01 cycles h^?1) temporal variability of ecological properties throughout the bay.  相似文献   

Cooling in rifting sequences during increasing burial depth due to heat flow decrease     

Andrea Ceriani  Andrea Di Giulio  Roberto Fantoni  Paolo Scotti 《地学学报》2006,18(5):365-371

Two case histories are presented to give evidences for sediment cooling during increasing burial depth due to heat flow decrease at the end of crustal stretching in extensional settings. The first refers to the Lower Cretaceous succession accumulated in a strongly subsiding trough within the Sirt Basin (Libya); the second relates to the Mesozoic succession of the Lombardian Basin (NW Italy) formed during Late Triassic–Early Jurassic rifting of the northern margin of the Adriatic microplate. In both cases, heat flow decreasing at the end of crustal stretching overbalanced the thermal effect of increasing burial depth causing a net cooling of rocks. These examples provide an alternative to exhumation for explaining cooling events recorded by rifting sedimentary sequences.  相似文献