activity
20002012
most citedProperties of the ionized gas in HH202. II: Results from echelle spectrophotometry with UVES

108 citations · 169 across the 16 of their papers we have counts for

collaborators
Showing 2003Show all

6 papers · 1 filter

astro-ph2003

The effect of collisional enhancement of Balmer lines on the determination of the primordial helium abundance

V. Luridiana, A. Peimbert, M. Peimbert +1

This paper describes a new determination of the primordial helium abundance (Y_P), based on the abundance analysis of five metal-poor extragalactic HII regions. For three regions o…

astro-ph2003

Physical limits to the validity of synthesis models: The Lowest Luminosity Limit

M. Cervino, V. Luridiana

(abriged) In this paper we establish a Lowest Luminosity Limit (LLL) for the use of synthesis codes. The limit is defined by the following statement: The total luminosity of the cl…

astro-ph2003

Physical conditions in NGC 6543 from ISO and HST data and the pitfalls of temperature maps

V. Luridiana, E. Perez, M. Cervino

We determine the physical conditions in NGC 6543, obtaining two different estimates of the electron temperature (T_e) and one estimate of the electron density (N_e). The electron t…

astro-ph20031 cited

Photoionization Models of Metal-poor Extragalactic HII Regions and the Primordial Helium Abundance

V. Luridiana, A. Peimbert, M. Peimbert

We discuss the effects of collisional enhancement of Balmer lines on the determination of the primordial helium abundance. To this aim, we present a photoionization model of the me…

astro-ph2003

Statistical Synthesis Models

M. Cervino, V. Luridiana

In this contribution we evaluate the minimal cluster mass for which the effects of an incomplete sampling of the Initial Mass Function (IMF) cannot be neglected. This minimal clust…

astro-ph2003

Physical conditions in the O++ zone from ISO and HST data. NGC 6543 revisited

V. Luridiana, E. Perez, M. Cervino

We revise the physical conditions in the O++ zone of the planetary nebula NGC 6543, obtaining two different estimates of the electron temperature (Te) and one estimate of the elect…