Minor Planet Observations [304 Las Campanas Observatory]
Not Available
Benecchi, S. et al.
Advertised on:
6
2010
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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Massive star formation in Wolf-Rayet galaxies. III. Analysis of the O and WR populationsAims: We perform a comprehensive multiwavelength analysis of a sample of 20 starburst galaxies that show a substantial population of Wolf-Rayet (WR) stars. In this paper, the third of the series, we present the analysis of the O and WR star populations within these galaxies. Methods: We study the spatial localization of the WR-rich clusters via theLópez-Sánchez, Á. R. et al.
Advertised on:
62010 -
Magnetic Field Structures and Turbulent Components in the Star-forming Molecular Clouds OMC-2 and OMC-3The SCUBA polarized 850 μm thermal emission data of the OMC-2 region in Orion A are added to and homogeneously reduced with data already available in the OMC-3 region. The data set shows that OMC-2 is a region generally less polarized than OMC-3. Where coincident, most of the 850 μm polarization pattern is similar to that measured in 350 μmPoidevin, F. et al.
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62010 -
Lunar single-scattering, porosity, and surface-roughness characteristics with SMART-1/AMIENot AvailableNäränen, J. et al.
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62010 -
Limits on Light-Speed Anisotropies from Compton Scattering of High-Energy ElectronsThe possibility of anisotropies in the speed of light relative to the limiting speed of electrons is considered. The absence of sidereal variations in the energy of Compton-edge photons at the European Synchrotron Radiation Facility’s GRAAL facility constrains such anisotropies representing the first nonthreshold collision-kinematics study ofBocquet, J.-P. et al.
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62010 -
Lightcurves of 6 Jupiter Trojan asteroidsFrom the point of view of the intrinsic rotation, the Jupiter Trojans are not as well characterized as the main belt asteroids, primarily because the available sample of lightcurves is small and mainly restricted to the largest objects. We have obtained rotational periods and lightcurve amplitudes for 6 Trojan asteroids, which range between valuesMelita, M. D. et al.
Advertised on:
62010