An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent von Pietrzyński, G., Graczyk, D., Gieren, W., Thompson, I. B., Pilecki, B., Udalski, A., Soszyński, I., Kozłowski, S., Konorski, P., Suchomska, K., Bono, G., Moroni, P. G. Prada, Villanova, S., Nardetto, N., Bresolin, F., Kudritzki, R. P., Storm, J., Gallenne, A., Smolec, R., Minniti, D., Kubiak, M., Szymański, M. K., Poleski, R., Wyrzykowski, Ł., Ulaczyk, K., Pietrukowicz, P., Górski, M., Karczmarek, P.

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Slowly fading super-luminous supernovae that are not pair-instability explosions von Nicholl, M., Smartt, S. J., Jerkstrand, A., Inserra, C., McCrum, M., Kotak, R., Fraser, M., Wright, D., Chen, T.-W., Smith, K., Young, D. R., Sim, S. A., Valenti, S., Howell, D. A., Bresolin, F., Kudritzki, R. P., Tonry, J. L., Huber, M. E., Rest, A., Pastorello, A., Tomasella, L., Cappellaro, E., Benetti, S., Mattila, S., Kankare, E., Kangas, T., Leloudas, G., Sollerman, J., Taddia, F., Berger, E., Chornock, R., Narayan, G., Stubbs, C. W., Foley, R. J., Lunnan, R., Soderberg, A., Sanders, N., Milisavljevic, D., Margutti, R., Kirshner, R. P., Elias-Rosa, N., Morales-Garoffolo, A., Taubenberger, S., Botticella, M. T., Gezari, S., Urata, Y., Rodney, S., Riess, A. G., Scolnic, D., Wood-Vasey, W. M., Burgett, W. S., Chambers, K., Flewelling, H. A., Magnier, E. A., Kaiser, N., Metcalfe, N., Morgan, J., Price, P. A., Sweeney, W., Waters, C.

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THE ARAUCARIA PROJECT: AN ACCURATE DISTANCE TO THE LATE-TYPE DOUBLE-LINED ECLIPSING BINARY OGLE SMC113.3 4007 IN THE SMALL MAGELLANIC CLOUD von GRACZYK, Dariusz, PIETRZYNSKI, Grzegorz, KONORSKI, Piotr, MENNICKENT, Ronald, MINNITI, Dante, STORM, Jesper, NARDETTO, Nicolas, KARCZMAREK, Paulina, THOMPSON, Ian B, GIEREN, Wolfgang, PILECKI, Bogumił, UDALSKI, Andrzej, SOSZYNSKI, Igor, KOLACZKOWSKI, Zbigniew, KUDRITZKI, Rolf-Peter, BRESOLIN, Fabio

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Chemical abundances and winds of massive stars in M31: a B-type supergiant and a WC star in OB 10 von Smartt, S.J., Crowther, P.A., Dufton, P.L., Lennon, D.J., Kudritzki, R.P., Herrero, A., McCarthy, J.K., Bresolin, F.

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Atmospheres and Winds of PN Central Stars von Kudritzki, R.P., Urbaneja, M.A., Puls, J.

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Chemical abundances and winds of massive stars in M31: a B-type supergiant and a WC star in OB 10 von Smartt, S.J., Crowther, P.A., Dufton, P.L., Lennon, D.J., Kudritzki, R.P., Herrero, A., McCarthy, J.K., Bresolin, F.

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A supergiants von Przybilla, N., Bresolin, F., Butler, K., Kaufer, A., Kudritzki, R.P., Venn, K.A.

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Hunting For Massive Late-Type Stars In The Inner Disk Of The Milky Way von Messineo, M., Zhu, Q., Menten, K.M., Ivanov, V.D., Figer, D.F., Habing, H.J., Kudritzki, R.P., Chen, C.H.R., Davies, B., Churchwell, E.

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Hunting For Massive Late-Type Stars In The Inner Disk Of The Milky Way von Messineo, M., Zhu, Q., Menten, K.M., Ivanov, V.D., Figer, D.F., Habing, H.J., Kudritzki, R.P., Chen, C.H.R., Davies, B., Churchwell, E.

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Evolutionary versus dynamical time scales for the evolution of the central stars of planetary nebulae von McCarthy, J. K., Mould, J. R., Mendez, R. H., Kudritzki, R. P., Husfeld, D., Herrero, A., Groth, H. G.

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Intrinsic Parameters of Hot Blue Stars von Kudritzki, R.P., Hummer, D.G.

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Model Atmospheres of Central Stars of PN von Kudritzki, R.P., Méndez, R.H.

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Non-LTE Analysis of Massive Stars in the Magellanic Clouds von Gehren, T., Husfeld, D., Kudritzki, R.P., Conti, P.S., Hummer, D.G.

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A source for mass-loss instabilities in LBV’s – the case of P Cygni von Pauldrach, A.W.A., Puls, J., Kudritzki, R.P.

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The wind of P Cygni von Puls, J., Pauldrach, A.W.A., Kudritzki, R.P.

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Winds of Hot Stars as a Diagnostic Tool of Stellar Evolution von Kudritzki, R.P., Pauldrach, A., Puls, J.

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The atmosphere of subluminous B stars von Heber, U., Hunger, K., Jonas, G., Kudritzki, R.P.

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Non-LTE analysis of central stars von Kudritzki, R.P., Méndez, R.H., Simon, K.P.

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Helium Rich Subdwarf O Stars and Central Stars of Planetary Nebulae von Méndez, R.H., Miguel, C.H., Heber, U., Kudritzki, R.P.

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NLTE analysis of SDO stars von Heber, U., Hunger, K., Kudritzki, R.P., Simon, K. P.

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