activity
20122019
most citedAn approach to effective temperature and surface gravity in post-AGB and RV Tauri stars at the near-IR region

3 citations · 6 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2019★ 1 cited

Chemical composition of post-AGB star candidates

R. E. Molina, C. B. Pereira, A. Arellano Ferro

We present a high resolution detailed abundance analysis for a sample of six post-AGB candidate stars, five of them had not been studied spectroscopically in the optical region. Al…

astro-ph.SR2018

Determination of stellar atmospheric parameters for a sample of the post-AGB stars

R. E. Molina

We report for the first time the stellar atmospheric parameters for a a set of post-AGB stars classified by Suarez et al. (2006). The stellar spectra were taken from optical region…

astro-ph.SR2016

Chemical abundances for A-and F-type supergiant stars

R. E. Molina, H. Rivera

We present the stellar parameters and elemental abundances of a set of A--F-type supergiant stars HD\,45674, HD\,180028, HD\,194951 and HD\,224893 using high resolution (\,$\sim…

astro-ph.SR2014★ 2 cited

Spectroscopic analysis of four post-AGB candidates

R. E. Molina, S. Giridhar, C. B. Pereira +2

We have done a detailed abundance analysis of four unexplored candidate post- Asymptotic Giant Branch(AGB) stars IRAS 13110 - 6629, IRAS 17579 - 3121, IRAS 18321 - 1401 and IRAS 18…

astro-ph.SR2013

Detailed atmospheric abundance analysis of the optical counterpart of the IR source IRAS 16559-2957

R. E. Molina, A. Arellano Ferro

We have undertaken a detailed abundance analysis of the optical counterpart of the IR source IRAS16559-2957 with the aim of confirming its possible post-AGB nature. The star shows…

astro-ph.SR2012★ 3 cited

An approach to effective temperature and surface gravity in post-AGB and RV Tauri stars at the near-IR region

R. E. Molina

A number of empirical correlations that allows us to calculate the effective temperature and surface gravity for a set evolved post-AGB and RV Tauri stars are determined using as c…