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The elusive origin of Carbon-Enhanced Metal-Poor stars
C. Abate, O. R. Pols, R. G. Izzard +2
Carbon-enhanced metal-poor (CEMP) stars count for 9-25% of all the very metal-poor stars of the halo. In at least some CEMP stars the chemical enrichment is believed to be due to w…
Unexpectedly large mass loss during the thermal pulse cycle of the red giant R Sculptoris!
M. Maercker, S. Mohamed, W. H. T. Vlemmings +10
The asymptotic giant branch star R Sculptoris is surrounded by a detached shell of dust and gas. The shell originates from a thermal pulse during which the star undergoes a brief p…
Herschel's view into Mira's head
A. Mayer, A. Jorissen, F. Kerschbaum +9
Herschel's PACS instrument observed the environment of the binary system Mira Ceti in the 70 and 160 micron bands. These images reveal bright structures shaped as five broken arcs…