Chemical Evolution of Super Star Clusters in a Positive Star Formation Feedback Scenario
Not Available
Mollá, M. et al.
Advertised on:
9
2014
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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Chemical Thermodynamics Applied to the Diels–AlderReaction of C60 Fullerene with Polyacenes
The Diels–Alder addition reactions of a series of acenes (anthracene, 9,10-dimenthylanthracene, tetracene and pentacene) to C60 fullerene are next to equilibrium reactions and were analyzed using a classic chemical thermodynamics approach using group increment calculations. In the case of the C60/anthracene adducts and C60/dimethylanthracene
Cataldo F. et al.Advertised on:
92015 -
Chemistry and kinematics of stars in Local Group galaxies
Not Available
Battaglia, GiuseppinaAdvertised on:
92007 -
Chromospheric Lyman-alpha spectro-polarimeter (CLASP)
One of the biggest challenges in heliophysics is to decipher the magnetic structure of the solar chromosphere. The importance of measuring the chromospheric magnetic field is due to both the key role the chromosphere plays in energizing and structuring the outer solar atmosphere and the inability of extrapolation of photospheric fields to
Kano, Ryouhei et al.Advertised on:
92012 -
Chromospheric modelling in late-type dwarfs. II - CES observations of active and quiescent stars
The characteristics of the chromospheres of late-type dwarf stars were studied using the CoudeEchelle Spectrograph (CES) at ESO and the IUE. The study focused on the h and k Mg II lines of F and G dwarfs. The stability of the IUE spectra permitted calculations of averaged absorption features and the subtraction of the Mg II lines to leave intrinsic
Foing, B. H. et al.Advertised on:
91985 -
Chromospheric Rotational Modulation in Solar-Like Stars - Part Two - Multicomponent Modelling and Rotational Period of Alpha-Centauri from CAII H Spectroscopic Variability
The K1V late-type dwarf α Cen B has been monitored to search for spectroscopic variability in the Ca II H chromospheric line during its rotational period. The observations were made with the Coudé Echelle Spectrograph with the 1.4 Coudé Auxiliary Telescope at ESO, with spectral resolution 80000. Variability in flux up to 29 % and profile
Char, S. et al.Advertised on:
91993