Matsuura, M., J. Bernard-Salas, T. Lloyd Evans, K. M. Volk, B. J. Hrivnak, G. C. Sloan, Y.-H. Chu, R. Gruendl, K. E. Kraemer, E. Peeters, R. Szczerba, P. R. Wood, A. A. Zijlstra, S. Hony, Y. Ita, D. Kamath, E. Lagadec, Q. A. Parker, W. A. Reid, T. Shimonishi, H. Van Winckel, P. M. Woods, F. Kemper, M. Meixner, M. Otsuka, R. Sahai, B. A. Sargent, J. L. Hora and I. McDonald: Spitzer Space Telescope spectra of post-AGB stars in the Large Magellanic Cloud - polycyclic aromatic hydrocarbons at low metallicities. In: Monthly Notices of the Royal Astronomical Society 439, 2, 1472-1493 (2014).
url: http://cdsads.u-strasbg.fr/abs/2014MNRAS.439.1472M
Oliveira, J. M., J. T. van Loon, G. C. Sloan, M. Sewilo, K. E. Kraemer, P. R. Wood, R. Indebetouw, M. D. Filipovic, E. J. Crawford, G. F. Wong, J. L. Hora, M. Meixner, T. P. Robitaille, B. Shiao and J. D. Simon: Early-stage young stellar objects in the Small Magellanic Cloud. In: Monthly Notices of the Royal Astronomical Society 428, 4, 3001-3033 (2013).
url: http://cdsads.u-strasbg.fr/abs/2012arXiv1210.5193O
Lebzelter, T., T. Posch, K. Hinkle, P. R. Wood and J. Bouwman: Tracing the development of dust around evolved stars: The case of 47 Tuc. 653, L145-L148 (2006).
url: http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006ApJ...653L.145L&db_key=AST
Woodruff, H. C., M. Eberhardt, T. Driebe, K.-H. Hofmann, K. Ohnaka, A. Richichi, D. Schertl, M. Schöller, M. Scholz, G. Weigelt, M. Wittkowski and P. R. Wood: Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared. In: Astronomy & Astrophysics 421, 2, 703-714 (2004).
Woodruff, H. C., M. Eberhardt, T. Driebe, K.-H. Hofmann, K. Ohnaka, A. Richichi, D. Schertl, M. Schöller, M. Scholz, G. Weigelt, M. Wittkowski and P. R. Wood: Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared. In: New Frontiers in Stellar Interferometry, (Eds.) Traub, W.A. Proceedings of SPIE 5491. SPIE, Bellingham (2004) 1707-1713.
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