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Context. Luminous blue variables (LBVs) are evolved massive stars that exhibit instabilities that are not yet understood. Stars can lose several solar masses during this evolutionary phase. The LBV phenomenon is thus critical to our understanding of the evolution of the most massive stars. Aims. ...


Mehner, A.Baade, D.Groh, J.H.Rivinius, T.Hambsch, F.-J.Bartlett, E.S.Asmus, D.Agliozzo, C.Szeifert, T.Stahl, O.[Spectroscopic and photometric oscillatory envelope variability during the S Doradus outburst of the luminous blue variable R71]Spectroscopic and photometric oscillatory envelope variability during the S Doradus outburst of the luminous blue variable R71

Ricci, ClaudioBauer, Franz Erik.Treister, Ezequiel.Nikutta, R.Assef T., RobertoStern, D.Alexander, D. M.Asmus, D.Ballantyne, D. R.Blain, A. W.Boggs, Steven E.[NuSTAR Observations of WISE J1036+0449, a Galaxy at z~1 Obscured by Hot Dust.]NuSTAR Observations of WISE J1036+0449, a Galaxy at z~1 Obscured by Hot Dust.
Lopez-Gonzaga, N.Asmus, D.Bauer, Franz Erik.Tristam, K.Burstcher, L.Marinucci, A.Matt, G.Harrison, F.[NGC 1068: No change in the mid-infrared torus structure despite X-ray variability]NGC 1068: No change in the mid-infrared torus structure despite X-ray variability
Annuar, A.Alexander, D.Gandhi, P.Lansbury, G.Asmus, D.Ballantyne, D.Bauer, Franz ErikBoggs, S.Boorman, P.Brandt W.Brightman, M.|Christensen, F.Craig, W.Farrah, D.Goulding, A.Hailey, C.Harrison, F.Koss, M.Lamassa, S.Murray, S.Ricci, C.Rosario, D.Stanley, F.Stern, D.Zhang, W.[A New Compton-thick AGN in Our Cosmic Backyard: Unveiling the Buried Nucleus in NGC 1448 with NuSTAR]A New Compton-thick AGN in Our Cosmic Backyard: Unveiling the Buried Nucleus in NGC 1448 with NuSTAR

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