activity
20002007
most citedCoordinated Multiwavelength Observations of BL Lacertae in 2000

78 citations · 131 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph2007★ 19 cited

A Spectroscopic Study of the Algol-type Binaries S Equulei and KO Aquilae: Absolute Parameters and Mass Transfer

F. Soydugan, A. Frasca, E. Soydugan +3

We present and analyze high-resolution optical spectra of the Algol binaries S Equ and KO Aql. New accurate radial velocities for the hotter primary components are obtained. Thanks…

astro-ph2007

Physical parameters of evolved stars in clusters and in the field from line-depth ratios

K. Biazzo, L. Pasquini, A. Frasca +6

We present a high-resolution spectroscopic analysis of two samples of evolved stars selected in the field and in the intermediate-age open cluster IC 4651, for which detailed measu…

astro-ph2007

Effective temperature vs line-depth ratio for ELODIE spectra. Gravity and rotational velocity effects

K. Biazzo, A. Frasca, S. Catalano +1

The dependence on the temperature of photospheric line-depth ratios (LDRs) in the spectral range 6190-6280 A is investigated by using a sample of 174 ELODIE Archive stellar spectra…

astro-ph2007★ 22 cited

Deriving temperature, mass and age of evolved stars from high-resolution spectra. Application to field stars and the open cluster IC 4651

K. Biazzo, L. Pasquini, L. Girardi +6

We test our capability of deriving stellar physical parameters of giant stars by analysing a sample of field stars and the well studied open cluster IC 4651 with different spectros…

astro-ph2006★ 1 cited

Spectroscopic Data Analysis for Precise Determination of Stellar Temperatures

K. Biazzo, A. Frasca, S. Catalano +1

The ratio of the depths of spectral lines is a powerful indicator of the effective temperature. The method based on this analysis is capable of discerning small temperature variati…

astro-ph2006★ 1 cited

Photospheric temperature measurements in young main sequence stars

K. Biazzo, A. Frasca, G. W. Henry +2

As part of our program to study stellar photospheric and chromospheric activity, we have examined several young solar type stars with activity levels intermediate between the Sun a…