A Theoretical Approach to the Estimate of Scattered Light into IUE Low Resolution Short Wavelength Spectra
Not Available
Crivellari, L. et al.
Advertised on:
11
1980
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 statistical analysis of Mg II h and k emission cores for variability in beta Hydri (G2 IV).Not AvailableBeckman, J. E. et al.
Advertised on:
111980 -
The nature of the Kleinmann-Low nebulaRecent data on, and interpretations of the Kleinmann-Low nebula are examined. It is suggested that associated high velocity gas is radiatively accelerated by a protostar in an early stage of premain-sequence contraction.Phillips, J. P. et al.
Advertised on:
101980 -
An automatic procedure for a determination of the effective temperature and gravity - Application to 100 O-type starsWe have developed an automatic procedure to determine Teff and log g from the comparison of observational data with their theoretical values. After a description of the method we compare our results for a sample of 100 O-type stars with the classifications of Conti and Walborn and with the determinations of Morrison by photometric indices. TheMorossi, C. et al.
Advertised on:
91980 -
Method for the determination of density and phase functions of interplanetary dustA method for the determination of the intensity of the solar light scattered by a unit volume of interplanetary space and thus the density and phase functions of interplanetary dust is presented. The method involves the calculation of the scattered light intensity as a function of sun-particle distance and elongation angle from a partly assumedMujica, A. et al.
Advertised on:
71980 -
Parasite light effects in International Ultraviolet Explorer (IUE) low resolution spectraProcedures were developed for extracting low resolution spectra while correcting for halation effects and scattered light within the instrument. To correct for halation, the spectra were extracted from the line-by-line images. Perpendicular scans of the image were fitted using an iterative least squares procedure with a known form function. TheCrivellari, L. et al.
Advertised on:
41980