Comet Observations [461 JATE Asteroid Survey, Piszkesteto Stn. (Konkoly)]
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Sarneczky, K. et al.
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12
2003
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Book Review: Galaxies at high redshift / I. Pérez-Fournon, M. Balcells, F. Moreno-Insertis, F. Sánchez (eds.). Cambridge, Cambridge University Press, XV+275 pp., 2003, ISBN 0-521-82591-1Not AvailablePérez-Fournon, I. et al.
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Bar-Driven Galaxy Evolution at Intermediate RedshiftsNon-axisymmetric features such as bars drive the dynamical and secular evolution of disk galaxies by exerting gravitational torques which redistribute mass and angular momentum. While most (> 70 %) spirals are barred in the local Universe, early studies of the Hubble Deep Field (HDF) suggest a remarkably low bar fraction ( 20 %) at intermediateJogee, S. et al.
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122003 -
An Empirical Criterion to Classify T Tauri Stars and Substellar Analogs Using Low-Resolution Optical SpectroscopyWe have compiled and studied photometric and spectroscopic data published in the literature of several star-forming regions and young open clusters (Orion, Taurus, IC 348, Sco-Cen complex, Chamaeleon I, TW Hydrae association, σ Orionis cluster, IC 2391, α Persei cluster, and the Pleiades). Our goal was to seek the definition of a simple empiricalMartín, E. L. et al.
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122003 -
A superburst from 4U 1254-69We report the detection with the BeppoSAX Wide Field Cameras of a superburst from 4U 1254-69. The superburst is preceded by a normal type-I X-ray burst, has a decay time that is the longest of all eight superbursts detected so far and a peak luminosity that is the lowest. Like for the other seven superbursts, the origin is a well-known type-I X-rayin't Zand, J. J. M. et al.
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A Search for Kinematic Evidence of Tidal Tails in Globular ClustersRecent star count surveys of areas around globular star clusters have shown strong evidence of tidal tails stretching out many degrees beyond the cluster tidal radius. These tails are believed to be cluster stars which have escaped due to tidal shocking after passages through the disk of the Galaxy. Although the statistical star counts indicate andLauchner, A. et al.
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122003