Visual Spectroscopy of R Scuti (Poster abstract)

Volume 43 number 1 (2015)

Lucian Undreiu

121 Beverly Avenue, Wise, VA 24293; lundreiu@hotmail.com

Andrew Chapman

Address correspondence to L. Undreiu, 121 Beverly Avenue, Wise, VA 24293; lundreiu@hotmail.com

Abstract

(Abstract only) We are currently conducting a visual spectral analysis of the brightest known RV Tauri variable star, R Scuti. The goal of our undergraduate research project is to investigate this variable star’s erratic nature by collecting spectra at different times in its cycle. Starting in late June of 2014 and proceeding into the following four months, we have monitored the alterations in the spectral characteristics that accompany the progression of R Sct’s irregular cycle. During this time, we were given the opportunity to document the star’s most recent descent from maximum brightness V~5 to a relatively deep minimum of V~7.5. Analysis of the data taken during the star’s period of declining magnitude has provided us with several interesting findings that concur with the observations of more technically sophisticated studies. Following their collection, we compared our observations and findings with archived material in the hopes of facilitating a better understanding of the physical state of RV Tauri stars and the perplexing nature of their evolution. Although identification of the elements in the star’s bright phase proved to be challenging, documenting clear absorption features in its fainter stage was far less difficult. As previously reported in similar studies, we identified prominent TiO molecular absorption bands near R Sct’s faintest state, typical of mid-M spectral type stars. In addition to these TiO absorption lines, we report the presence of many more metallic lines in the spectral profiles obtained near star’s minimum. Supportive of previously published hypotheses regarding the causation of its variability, we observed significant variation in the star’s spectral characteristics throughout different phases of its cycle. We are hopeful that our observations will make a meaningful contribution to existing databases and help advance our collective understanding of RV Tauri stars and their evolutionary significance.