天下博览::文章
<a href="http://arxiv.org/find/astro-ph/1/au:+Hales_A/0/1/0/all/0/1">Antonio S. Hales</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barlow_M/0/1/0/all/0/1">Michael J. Barlow</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Drew_J/0/1/0/all/0/1">Jan | 2009年01月09日 11:17:32
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We have identified 17 A-type stars in the Galactic Plane that have mid-IRexcesses at 8 micron. From the observed colors in the (...
<a href="http://arxiv.org/find/astro-ph/1/au:+Bhadra_A/0/1/0/all/0/1">Arunava Bhadra</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ghosh_S/0/1/0/all/0/1">Sanjay K. Ghosh</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Joarder_P/0/1/0/all/0/1">Part | 2009年01月09日 11:17:32
We study low energy hadronic interaction models based on BESS observed cosmicray proton and antiproton spectra at medium high al...
<a href="http://arxiv.org/find/astro-ph/1/au:+Poleski_R/0/1/0/all/0/1">Radoslaw Poleski</a> | 2009年01月09日 11:17:32
Pulsation period of Cepheids should change as stars evolve through theinstability strip. Rates of these changes found by other a...
<a href="http://arxiv.org/find/astro-ph/1/au:+Diaferio_A/0/1/0/all/0/1">Antonaldo Diaferio</a> | 2009年01月09日 11:17:32
Traditional estimators of the mass of galaxy clusters assume that the clustercomponents (galaxies, intracluster medium, and dark...
<a href="http://arxiv.org/find/astro-ph/1/au:+Longcope_D/0/1/0/all/0/1">Dana Longcope</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Parnell_C/0/1/0/all/0/1">Clare Parnell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+DeForest_C/0/1/0/all/0/1">Cr | 2009年01月09日 11:17:32
Magnetic null points can be located numerically in a potential fieldextrapolation or their average density can be estimated from...
<a href="http://arxiv.org/find/astro-ph/1/au:+Parkin_E/0/1/0/all/0/1">E. R. Parkin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pittard_J/0/1/0/all/0/1">J. M. Pittard</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Corcoran_M/0/1/0/all/0/1">M. F. | 2009年01月09日 11:17:32
The X-ray emission from the super-massive star Eta Carinae is simulated usinga three dimensional model of the wind-wind collisio...
<a href="http://arxiv.org/find/astro-ph/1/au:+Horne_K/0/1/0/all/0/1">Keith Horne</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Snodgrass_C/0/1/0/all/0/1">Colin Snodgrass</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tsapras_Y/0/1/0/all/0/1">Yian | 2009年01月09日 11:17:32
OGLE III and MOA II are discovering 600-1000 Galactic Bulge microlens eventseach year. This stretches the resources available fo...
<a href="http://arxiv.org/find/astro-ph/1/au:+Krause_M/0/1/0/all/0/1">Marita Krause</a> | 2009年01月09日 11:17:32
From our radio observations of the magnetic field strength and large-scalepattern of spiral galaxies of different Hubble types a...
<a href="http://arxiv.org/find/astro-ph/1/au:+Petrovay_K/0/1/0/all/0/1">K. Petrovay</a> | 2009年01月09日 11:17:32
While obviously having a common root, solar and planetary dynamo theory havetaken increasingly divergent routes in the last two ...
<a href="http://arxiv.org/find/astro-ph/1/au:+Bonatto_C/0/1/0/all/0/1">Charles Bonatto</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bica_E/0/1/0/all/0/1">Eduardo Bica</a> | 2009年01月09日 11:17:32
The very young open cluster (OC) NGC 2244 in the Rosette Nebula was studiedwith field-star-decontaminated 2MASS photometry, whic...
