------------------------------------------------------------------------ granularity.tex ApJL accepted, Feb 2006 MIME-Version: 1.0 Content-Type: text/plain; charset=UTF-8 Content-Disposition: inline X-MailScanner-Information: Please contact postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (score=0, required 5, autolearn=disabled) X-MailScanner-From: ajgosling@gmail.com Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from base64 to 8bit by dropbox.aoc.nrao.edu id k2DB4wx3026792 %astro-ph/0602410 \documentclass[12pt,preprint]{aastex} \usepackage{emulateapj5,graphics} %emulateapj5,graphics,natbib, %%%%%%%%%%%%%%%%%%%%%%%%% %\newcommand{\arcsec}{^{\prime\prime}} \newcommand{\ks}{K_{\rm s}} \renewcommand{\floatpagefraction}{0.9} \renewcommand{\textfraction}{0.00} \newcommand{\vdag}{(v)^\dagger} \newcommand{\myemail}{ajg@astro.ox.ac.uk} \newcommand{\gtsim}{\mbox {{\raisebox{-0.4ex}{$\stackrel{>}{{\scriptstyle\sim}}$}}}} \newcommand{\ltsim}{\mbox {{\raisebox{-0.4ex}{$\stackrel{<}{{\scriptstyle\sim}}$}}}} \newcommand{\mc}{\multicolumn} %% You can insert a short comment on the title page using the command below. %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \slugcomment{Draft of \today} \shorttitle{Granular Extinction in the Galactic Centre} \shortauthors{Gosling, Blundell \& Bandyopadhyay} \begin{document} \title{Complex small-scale structure in the infrared extinction towards the Galactic Centre} \author{Andrew J.\ Gosling\altaffilmark{1}, Katherine M.\ Road, Oxford, OX1 3RH, U.K.} \begin{abstract} A high level of complex structure, or ``granularity'', has been observed in the distribution of infrared-obscuring material towards the Galactic Centre (GC), with a characteristic scale of $5\arcsec - 15\arcsec$, corresponding to $0.2 - 0.6\,{\rm pc}$ at a GC distance of $8.5\,{\rm kpc}$. This structure has been observed in ISAAC images which have a resolution of $\sim0.6\arcsec$, significantly higher than that of previous studies of the GC. We have discovered granularity throughout the GC survey region, which covers an area of $1.6^{\circ} \times 0.8^{\circ}$ in longitude and latitude respectively ($300\,{\rm pc} \times 120\,{\rm pc}$ at $8.5\,{\rm kpc}$) centred on Sgr A*. This granularity is variable over the whole region, with some areas exhibiting highly structured extinction in one or more wavebands and other areas displaying no structure and a uniform stellar distribution in all wavebands. The granularity does not appear to correspond to longitude, latitude or radial distance from Sgr A*. We find that regions exhibiting high granularity are strongly associated with high stellar reddening. \end{abstract} \keywords{dust, extinction---Galaxy: center---infrared: stars---ISM: structure} \end{document} On 21/02/06, Jennifer & Joseph wrote: > Hello, > > I saw this paper on astro-ph. If you haven't already done so, please > don't forget to submit it to GCNews, http://www.aoc.nrao.edu/~gcnews/ >, the newsletter for Galactic center > research. > > Thanks, > > -- Joseph > > > -- --------------------------------------------------------------------- Andrew Gosling ajgosling@gmail.com MCR Social Sec ajg@astro.ox.ac.uk Hertford College andrew.gosling@hertford.ox.ac.uk Oxford