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20112017
most citedThe VLTI/MIDI view on the inner mass loss of evolved stars from the Herschel MESS sample

26 citations · 54 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2017★ 26 cited

The VLTI/MIDI view on the inner mass loss of evolved stars from the Herschel MESS sample

C. Paladini, D. Klotz, S. Sacuto +12

The mass-loss process from evolved stars is a key ingredient for our understanding of many fields of astrophysics, including stellar evolution and the chemical enrichment of the in…

astro-ph.SR2016

Identifying the chemistry of the dust around AGB stars in nearby galaxies

Sundar Srinivasan, Franciska Kemper, Ronny Zhao-Geisler

Asymptotic giant branch (AGB) stars are significant contributors to the chemical enrichment of the interstellar medium (ISM) of galaxies. It is therefore essential to constrain the…

astro-ph.GA2016

The interstellar dust reservoir: SPICA's view on dust production and the interstellar medium in galaxies

F. Kemper, R. Zhao-Geisler, O. C. Jones +1

Typical galaxies emit about one third of their energy in the infrared. The origin of this emission reprocessed starlight absorbed by interstellar dust grains and reradiated as ther…

astro-ph.SR2015★ 1 cited

High-resolution CO observation of the carbon star CIT 6 revealing the spiral structure and a nascent bipolar outflow

Hyosun Kim, Sheng-Yuan Liu, Naomi Hirano +8

CIT 6 is a carbon star in the transitional phase from the asymptotic giant branch (AGB) to the protoplanetary nebulae (pPN). Observational evidences of two point sources in the opt…

astro-ph.GA2013★ 1 cited

Millimetric and sub-millimetric observations of IRAS 05327+3404 "Holoea" in M36

O. Morata, Y. J. Kuan, P. T. P. Ho +3

The transition between the proto-star, Class I, and the pre-main sequence star, Class II, phases is still one of the most uncertain, and important, stages in the knowledge of the p…

astro-ph.SR2011★ 26 cited

The mid-infrared diameter of W Hydrae

R. Zhao-Geisler, A. Quirrenbach, R. Koehler +2

Mid-infrared (8-13 microns) interferometric data of W Hya were obtained with MIDI/VLTI between April 2007 and September 2009, covering nearly three pulsation cycles. The spectrally…