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相关论文: A scaling law for interstellar depletions

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Dust infrared emission possesses scaling properties. Overall luminosity is never an input parameter of the radiative transfer problem, spectral shape is the only relevant property of the heating radiation when the inner boundary of the…

天体物理学 · 物理学 2015-06-24 Zeljko Ivezic , Moshe Elitzur

Ever since the pioneering work of Schmidt a half-century ago there has been great interest in finding an appropriate empirical relation that would directly link some property of interstellar gas with the process of star formation within it.…

星系天体物理 · 物理学 2015-06-23 Charles J. Lada

Scaling relations among galaxy cluster observables, which will become available in large future samples of galaxy clusters, could be used to constrain not only cluster structure, but also cosmology. We study the utility of this approach,…

宇宙学与河外天体物理 · 物理学 2015-05-13 Cien Shang , Zoltan Haiman , Licia Verde

We investigate the properties of Damped Lyman-alpha systems (DLAs) using high-resolution and large box-size cosmological hydrodynamical simulations of a LambdaCDM model. The numerical code used is a modification of GADGET-2 with a self…

宇宙学与河外天体物理 · 物理学 2015-05-13 Edoardo Tescari , Matteo Viel , Luca Tornatore , Stefano Borgani

Mineral dust aerosols impact Earth's radiation budget through interactions with clouds, ecosystems, and radiation, which constitutes a substantial uncertainty in understanding past and predicting future climate changes. One of the causes of…

大气与海洋物理 · 物理学 2011-01-20 Jasper F. Kok

We study the dust depletion pattern in eight well separated components of the z=1.973, logN(HI)=20.83, damped Lyman-alpha system toward Q0013-004, four of which have detectable H2 absorption. The apparent correlation between the abundance…

天体物理学 · 物理学 2009-11-07 Patrick Petitjean , R. Srianand , Cédric Ledoux

We revisit the main HI-to-stellar mass ratio (gas fraction) scaling relations, taking advantage of the HI spectral stacking technique to understand the dependence of gas content on the structural and star formation properties of nearby…

星系天体物理 · 物理学 2015-08-06 Toby Brown , Barbara Catinella , Luca Cortese , Virginia Kilborn , Martha P. Haynes , Riccardo Giovanelli

This article gives an overview of the constitution, physical conditions and observables of dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial distribution of dust in these objects, and its…

星系天体物理 · 物理学 2022-08-10 F. Galliano , M. Galametz , A. P. Jones

A recently proposed scaling law for the decay time of alpha particles is generalized for cluster decay. It is shown that for the decay of even-even parents, $logT_{1/2}$ depends linearly on the scaling variable…

核理论 · 物理学 2009-09-25 Mihai Horoi , B. Alex Brown , Aurel Sandulescu

We have collected data for 69 Damped Lyman-alpha (DLA) systems, to investigate the chemical evolution of galaxies in the redshift interval 0.0 < z < 4.4. In doing that, we have adopted the most general approach used so far to correct for…

天体物理学 · 物理学 2007-05-23 S. Savaglio , N. Panagia , M. Stiavelli

We present scaling laws for advection, radiation, magnetic drag and ohmic dissipation in the atmospheres of hot giant exoplanets. In the limit of weak thermal ionization, ohmic dissipation increases with the planetary equilibrium…

地球与行星天体物理 · 物理学 2015-05-30 Kristen Menou

ALMA Cycle 2 observations of the long wavelength dust emission in 145 star-forming galaxies are used to probe the evolution of star-forming ISM. We also develop the physical basis and empirical calibration (with 72 low-z and z ~ 2 galaxies)…

Medium modifications of parton fragmentation provide a novel tomographic tool for the study of the hot and dense matter created in ultrarelativistic nucleus-nucleus collisions. Their quantitative analysis, however, is complicated by the…

高能物理 - 唯象学 · 物理学 2008-11-26 Carlos A. Salgado , Urs Achim Wiedemann

We investigate the attenuation law in $z\sim 6$ quasars by combining cosmological zoom-in hydrodynamical simulations of quasar host galaxies, with multi-frequency radiative transfer calculations. We consider several dust models differing in…

星系天体物理 · 物理学 2021-07-21 F. Di Mascia , S. Gallerani , A. Ferrara , A. Pallottini , R. Maiolino , S. Carniani , V. D'Odorico

Interactions between dark matter and dark energy which result in a power-law behavior (with respect to the cosmic scale factor) of the ratio between the energy densities of the dark components (thus generalizing the LCDM model) have been…

宇宙学与河外天体物理 · 物理学 2012-06-14 David R. Castro , Hermano Velten , Winfried Zimdahl

The study of the interstellar medium (ISM) in the X-rays has entered a golden age with the advent of the X-ray observatories XMM-Newton and Chandra. High-energy resolution allowed to study dust spectroscopic features with unprecedented…

星系天体物理 · 物理学 2023-04-05 Elisa Costantini , Lia Corrales

We investigate the relationship between the dust-to-metals ratio (D/M) and the local interstellar medium environment at ~2 kpc resolution in five nearby galaxies: IC342, M31, M33, M101, and NGC628. A modified blackbody model with a broken…

To describe the small-scale intermittency of turbulence, a self-similarity is assumed for the probability density function of a logarithm of the rate of energy dissipation smoothed over a length scale among those in the inertial range. The…

流体动力学 · 物理学 2015-03-30 H. Mouri

The dust-to-metals ratio describes the fraction of the heavy elements contained in dust grains, and its variation provides key insights into the life cycle of dust. We measure the dust-to-metals ratio in M101, a nearby galaxy with a radial…

星系天体物理 · 物理学 2018-10-02 I-Da Chiang , Karin M. Sandstrom , Jérémy Chastenet , L. Clifton Johnson , Adam K. Leroy , Dyas Utomo

Compressed frictional granular matter cannot flow without dilation. Upon forced shearing to generate flow, the amount of dilation may depend on the initial preparation and a host of material variables. On the basis of both experiments and…