Herschel Observations of a Newly Discovered UX Ori Star in the Large Magellanic Cloud
Geoffrey C. Clayton, B. Sargent, M.L. Boyer, B. A. Whitney, Jacco Th., van Loon, M. Meixner, P. Tisserand, C. Engelbracht, S. Hony, R. Indebetouw,, K. A. Misselt, K. Okumura, P. Panuzzo, J. Roman-Duval, M. Sauvage, J. M., Oliveira, M. Sewilo, and E. Churchwell

TL;DR
This paper reports the discovery and analysis of a new UX Ori star in the Large Magellanic Cloud, characterized by irregular brightness variations, IR excess, and a circumstellar dust environment, expanding the known population of such stars.
Contribution
It presents the first detailed observation and modeling of a UX Ori star in the LMC, including its spectral features and circumstellar dust structure, highlighting its significance as only the second such star found there.
Findings
Displays irregular brightness drops up to 2 mag with reddening and blueing.
Spectral analysis shows emission and absorption lines typical of UX Ori stars.
SED modeling indicates a dusty disk and extended envelope around the star.
Abstract
The LMC star, SSTISAGE1C J050756.44-703453.9, was first noticed during a survey of EROS-2 lightcurves for stars with large irregular brightness variations typical of the R Coronae Borealis (RCB) class. However, the visible spectrum showing emission lines including the Balmer and Paschen series as well as many Fe II lines is emphatically not that of an RCB star. This star has all of the characteristics of a typical UX Ori star. It has a spectral type of approximately A2 and has excited an H II region in its vicinity. However, if it is an LMC member, then it is very luminous for a Herbig Ae/Be star. It shows irregular drops in brightness of up to 2 mag, and displays the reddening and "blueing" typical of this class of stars. Its spectrum, showing a combination of emission and absorption lines, is typical of a UX Ori star that is in a decline caused by obscuration from the circumstellar…
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
