SIMBAD references

2008MNRAS.387.1335R - Mon. Not. R. Astron. Soc., 387, 1335-1343 (2008/July-1)

Towards the main sequence: detailed analysis of weak line and post-T Tauri stars.

ROJAS G., GREGORIO-HETEM J. and HETEM A.Jr

Abstract (from CDS):

A detailed study was performed for a sample of low-mass pre-main-sequence (PMS) stars, previously identified as weak-line T Tauri stars, which are compared to members of the Tucanae and Horologium Associations. Aiming to verify if there is any pattern of abundances when comparing the young stars at different phases, we selected objects in the range from 1 to 100 Myr, which covers most of PMS evolution. High-resolution optical spectra were acquired at European Southern Observatory and Observatório do Pico dos Dias. The stellar fundamental parameters effective temperature and gravity were calculated by excitation and ionization equilibria of iron absorption lines. Chemical abundances were obtained via equivalent width calculations and spectral synthesis for 44 per cent of the sample, which shows metallicities within 0.5 dex solar. A classification was developed based on equivalent width of LII 6708 Å and Hα lines and spectral types of the studied stars. This classification allowed a separation of the sample into categories that correspond to different evolutive stages in the PMS. The position of these stars in the Hertzsprung-Russell diagram was also inspected in order to estimate their ages and masses. Among the studied objects, it was verified that our sample actually contains seven weak-line T Tauri stars, three are Classical T Tauri, 12 are Fe/Ge PMS stars and 21 are post-T Tauri or young main-sequence stars. An estimation of circumstellar luminosity was obtained using a disc model to reproduce the observed spectral energy distribution. Most of the stars show low levels of circumstellar emission, corresponding to less than 30 per cent of the total emission.

Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): stars: abundances - circumstellar matter - stars: fundamental parameters - stars: pre-main-sequence

CDS comments: Stars PDS 171, 177, 181, 330, 390S, 401, 390 are not identified.

Simbad objects: 44

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2008MNRAS.387.1335R and select 'bookmark this link' or equivalent in the popup menu


2019.10.19-00:38:26

© Université de Strasbourg/CNRS

    • Contact