activity
20162020
most citedOrganic molecules, ions, and rare isotopologues in the remnant of the stellar-merger candidate, CK Vulpeculae (Nova 1670)

32 citations · 32 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2020

Rotational spectra of vibrationally excited AlO and TiO in oxygen rich stars

T. Danilovich, C. A. Gottlieb, L. Decin +6

Rotational transitions in vibrationally excited AlO and TiO -- two possible precursors of dust -- were observed in the 300 GHz range (1 mm wavelength) towards the oxygen rich AGB s…

astro-ph.SR2019

Astro2020 Science White Paper: The fundamentals of outflows from evolved stars

E. De Beck, M. L. Boyer, V. Bujarrabal +16

Models of the chemical evolution of the interstellar medium, galaxies, and the Universe rely on our understanding of the amounts and chemical composition of the material returned b…

astro-ph.SR2018

Submillimeter-wave emission of three Galactic red novae: cool molecular outflows produced by stellar mergers

T. Kaminski, W. Steffen, R. Tylenda +3

Red novae are optical transients erupting at luminosities typically higher than those of classical novae. Their outbursts are believed to be caused by stellar mergers. We present m…

astro-ph.SR2018

Widespread HCN maser emission in carbon-rich evolved stars

K. M. Menten, F. Wyrowski, D. Keller +1

Context. HCN is a major constituent of the circumstellar envelopes of carbon-rich evolved stars, and rotational lines from within its vibrationally excited states probe parts of th…

astro-ph.SR201732 cited

Organic molecules, ions, and rare isotopologues in the remnant of the stellar-merger candidate, CK Vulpeculae (Nova 1670)

T. Kamiński, K. M. Menten, R. Tylenda +3

CK Vul is a star whose outburst was observed in 1670-72. A stellar-merger event was proposed to explain its ancient eruption. Aims: We aim to investigate the composition of the mol…

astro-ph.SR2016

Resolving the extended atmosphere and the inner wind of Mira ( Ceti) with long ALMA baselines

K. T. Wong, T. Kamiński, K. M. Menten +1

The prototypical Mira variable, Cet (Mira), has been observed as a Science Verification target in the 2014 ALMA Long Baseline Campaign with a longest baseline of 15 km. ALMA cl…