A composite HII region luminosity function (Bradley+, 2006)
HII region catalogues for 57 face on spiral galaxies within v
Bradley, T. R. et al.
Advertised on:
9
2006
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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A continuous follow-up of Centaurs, and dormant comets: looking for cometary activity.MOTIVATION FOR THIS MONITORING To better understand the origin, nature and evolution of the Kuiper Belt Objects (hereafter KBOs) it is needed a characterization of the physical properties of these primitive bodies. We expect that these remote and pristine bodies are rich in ice and other volatiles. They also probably played an important role in theTrigo-Rodríguez, J. M. et al.
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92008 -
A coordinated campaign of the intermediate polar AE aqr. 1: The system parametersWe report intermediate resolution spectroscopy (50 km/s) of the magnetic Cataclysmic Variable AE Aqr performed as part of the World Astronomy Days (WAD) campaign. Our analysis of the absorption features supports a K4 classification for the companion star, which contributes more than 95% of the total flux in the range 600-700 nm. We find that theCasares, J. et al.
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91996 -
A deep look into the core of young clusters. II. λ-OrionisContext: Over the past years, the λ-Orionis cluster has been a prime location for the study of young very low mass stars, substellar and isolated planetary mass objects and the determination of the initial mass function and other properties of low mass cluster members. Aims: In the continuity of our previous studies of young associations cores, weBouy, H. et al.
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92009 -
A deep search for the host galaxies of gamma-ray bursts with no detected optical afterglowContext. Gamma-ray bursts (GRBs) can provide information about star formation at high redshifts. Even in the absence of a bright optical/near-infrared/radio afterglow, the high detection rate of X-ray afterglows by Swift/XRT and its localization precision of 2-3 arcsec facilitates the identification and the study of GRB host galaxies. Aims: WeRossi, A. et al.
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92012 -
A deep, precise determination of the substellar mass function and its radial dependence in the open cluster IC 2391 from a multiband optical-infrared surveyNot AvailableBoudreault, Steve et al.
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92007