# The SAGE-Spec Spitzer Legacy program: The life-cycle of dust and gas in   the Large Magellanic Cloud. Point source classification III

**Authors:** Olivia C. Jones, Paul M. Woods, F. Kemper, K. E. Kraemer, G. C. Sloan,, S. Srinivasan, J. M. Oliveira, J. Th. van Loon, Martha L. Boyer, Benjamin A., Sargent, I. McDonald, Margaret Meixner, A. A. Zijlstra, Paul M. E. Ruffle, E., Lagadec, Tyler Pauly, Marta Sewi{\l}o, G. C. Clayton, K. Volk

arXiv: 1705.02709 · 2017-07-26

## TL;DR

This study classifies nearly 800 infrared point sources in the Large Magellanic Cloud using Spitzer IRS spectra, revealing diverse stellar populations, dust properties, and catalog inconsistencies, thereby enhancing understanding of LMC's stellar and dust evolution.

## Contribution

Introduces a decision-tree spectral classification method for LMC point sources, refining classifications with literature data and revealing catalog contamination and incompleteness.

## Key findings

- YSO and HII regions dominate the sample
- Identification of rare stellar evolutionary types
- Detection of catalog contamination and missing sources

## Abstract

The Infrared Spectrograph (IRS) on the {\em Spitzer Space Telescope} observed nearly 800 point sources in the Large Magellanic Cloud (LMC), taking over 1,000 spectra. 197 of these targets were observed as part of the Sage-Spec Spitzer Legacy program; the remainder are from a variety of different calibration, guaranteed time and open time projects. We classify these point sources into types according to their infrared spectral features, continuum and spectral energy distribution shape, bolometric luminosity, cluster membership, and variability information, using a decision-tree classification method. We then refine the classification using supplementary information from the astrophysical literature. We find that our IRS sample is comprised substantially of YSO and H\,{\sc ii} regions, post-Main Sequence low-mass stars: (post-)AGB stars and planetary nebulae and massive stars including several rare evolutionary types. Two supernova remnants, a nova and several background galaxies were also observed. We use these classifications to improve our understanding of the stellar populations in the Large Magellanic Cloud, study the composition and characteristics of dust species in a variety of LMC objects, and to verify the photometric classification methods used by mid-IR surveys. We discover that some widely-used catalogues of objects contain considerable contamination and others are missing sources in our sample.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1705.02709/full.md

## Figures

46 figures with captions in the complete paper: https://tomesphere.com/paper/1705.02709/full.md

## References

175 references — full list in the complete paper: https://tomesphere.com/paper/1705.02709/full.md

---
Source: https://tomesphere.com/paper/1705.02709