Taking the waters, 1999-style     

Eric Robinson 《Geology Today》1999,15(2):79-80

  相似文献   

Mid-infrared, spatially resolved spectroscopy of the nucleus of the Circinus galaxy     

Patrick F. Roche  Christopher Packham  Charles M. Telesco  James T. Radomski  Almudena Alonso-Herrero  David K. Aitken  Luis Colina  Eric Perlman 《Monthly notices of the Royal Astronomical Society》2006,367(4):1689-1698

High spatial resolution spectroscopy at 8–13 μm with T-ReCS on Gemini-S has revealed striking variations in the mid-infrared emission and absorption in the nucleus of the Circinus galaxy (hereafter Circinus) on subarcsecond scales. The core of Circinus is compact and obscured by a substantial column of cool silicate dust. Weak extended emission to the east and west coincides with the coronal line region and arises from featureless dust grains which are probably heated by line emission in the coronal emission zone. The extended emission on the east side of the nucleus displays a much deeper silicate absorption than that on the west, indicating significant columns of cool material along the line of sight and corresponding to an additional extinction of   A_V ∼ 25 mag  . Emission bands from aromatic hydrocarbons are not subject to this additional extinction, are relatively weak in the core and in the coronal line region, and are much more spatially extended than the continuum dust emission; they presumably arise in the circumnuclear star-forming regions. These data are interpreted in terms of an inclined disc-like structure around the nucleus extending over tens of parsecs and possibly related to the inner disc found from observations of water masers by Greenhill et al..  相似文献   

Coronae & Outflows from Helical Dynamos, Compatibility with the MRI, and Application to Protostellar Disks     

Eric G. Blackman  Jonathan C. Tan 《Astrophysics and Space Science》2004,292(1-4):395-406

Magnetically mediated disk outflows are a leading paradigm to explain winds and jets in a variety of astrophysical sources, but where do the fields come from? Since accretion of mean magnetic flux may be disfavored in a thin turbulent disk, and only fields generated with sufficiently large scale can escape before being shredded by turbulence, in situ field production is desirable. Nonlinear helical inverse dynamo theory can provide the desired fields for coronae and outflows. We discuss the implications for contemporary protostellar disks, where the (magneto-rotational instability (MRI)) can drive turbulence in the inner regions, and primordial protostellar disks, where gravitational instability drives the turbulence. We emphasize that helical dynamos are compatible with the magneto-rotational instability, and clarify the relationship between the two.  相似文献   

Historical Notes: Bowerbank: a forgotten geologist     

Eric Robinson 《Geology Today》2003,19(6):219-222

  相似文献   

EURD observations of interstellar radiation     

Jerry Edelstein  Stuart Bowyer  Eric J. Korpela  Michael Lampton  JoaquÍn Trapero  José F. Gómez  Carmen Morales  Veronica Orozco 《Astrophysics and Space Science》2001,276(1):177-185

The hot interstellar medium (ISM) has far-reaching effect upon thestructure of galaxies. Although ISM heating processes are fairly wellunderstood, after decades of study, the processes that cool the hotinterstellar medium remain obscure. The EURD spectrograph was designed tomeasure the diffuse cosmic background from 350 to 1100 Å in order tostudy the hot ISM and the mechanisms by which it sheds its energy. Wepresent the first analysis of EURD observations of the cosmic background.These EURD observations have proven to be far more sensitive than previouswork; compared to previous results, we have improved the limits to theintensity of 450 to 900 Å line emission from the ISM by one to twoorders of magnitude. Our limit to OVI 1032 Å / 1038 Å doublet of 7900ph s^-1 cm^-2 str^-1 is the lowest yet reported. The EURDlimits to line emission are less intense than predicted by a varietytheoretical models of the local ISM.  相似文献   

Late glacial and Holocene vegetation history at Governor Bog,King Valley,western Tasmania,Australia     

Eric A. Colhoun  Guus van de Geer  Sean J. Fitzsimons 《第四纪科学杂志》1991,6(1):55-66

  相似文献   

New models of interstellar gas–grain chemistry – III. Solid CO₂     

Deborah P. Ruffle  Eric Herbst † 《Monthly notices of the Royal Astronomical Society》2001,324(4):1054-1062

Solid CO₂ is observed to be an abundant interstellar ice component towards both quiescent clouds and active star-forming regions. Our recent models of gas–grain chemistry, appropriate for quiescent regions, severely underproduce solid CO₂ at the single assumed gas density and temperature. In this paper, we investigate the sensitivity of our model results to changes in these parameters. In addition, we examine how the nature of the grain surface affects the results and also consider the role of the key surface reaction between O and CO. We conclude that the observed high abundance of solid CO₂ can be reproduced at reasonable temperatures and densities by models with diffusive surface chemistry, provided that the diffusion of heavy species such as O occurs efficiently.  相似文献   

WILLIAM BUCKLAND'S FRENCH MEGALOSAURUS     

Eric Buffetaut  Gilles Cuny  ré Pharisat 《地学学报》1994,6(3):323-326

  相似文献   

Nature and completeness of galaxies detected in the Two Micron All Sky Survey     

Daniel H. McIntosh  Eric F. Bell  Martin D. Weinberg  Neal Katz 《Monthly notices of the Royal Astronomical Society》2006,373(4):1321-1338

  相似文献   

Circumstellar Molecular Spectra Towards Evolved Stars     

Eric J. Bakker 《Astrophysics and Space Science》1997,251(1-2):73-80

In this paper we discuss the relevance, and possible scientific gains, which can be acquired from studying circumstellar molecular spectra toward evolved stars. Where can we expect circumstellar molecular spectra, why would we want to study these spectra, which molecules might be present, and what can we learn from these studies? We present an overview of reported detections, and discuss some of the results.  相似文献