Ute Lisenfeld
University of Granada
205 Papers
1.8K Citations
Ute Lisenfeld is an academic researcher from University of Granada. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 42, co-authored 191 publications. Previous affiliations of Ute Lisenfeld include Max Planck Society & Spanish National Research Council.
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Papers
The AMIGA sample of isolated galaxies: VII Far-infrared and radio continuum study of nuclear activity [complementary material]
J. Sabater,Stephane Leon,Lourdes Verdes-Montenegro,Ute Lisenfeld,Jack W. Sulentic,S. Verley +5 more
- 01 Jan 2008
TL;DR: The AMIGA project as discussed by the authors provided a statistically significant sample of the most isolated galaxies in the northern sky, where the authors used the well-known radio continuum-FIR correlation to select radio-excess galaxies that are candidates to host an active galactic nucleus (AGN), as well as the FIR colours to find obscured AGN-candidates.
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Distribution of the Extinction and Star Formation in NGC 1569
TL;DR: In this paper, the distribution of the intrinsic extinction in the starburst dwarf galaxy NGC1569 was investigated, and an extinction map of the whole galaxy derived from the Halpha/Hbeta emission line ratio was derived.
Molecular gas and dust in Arp 94: The formation of a recycled galaxy in an interacting system
TL;DR: In this article, the authors present new results for the molecular gas, dust emission and the ionized gas in J1023+1952, an HI rich intergalactic star-forming tidal dwarf galaxy candidate.
A 0.6 Mpc H i structure associated with Stephan’s Quintet
C. Cheng,P. N. Appleton,P. A. Duc,Yu Gao,Ning-Yu Tang,M. S. Yun,Y. S. Dai,J.-S. Huang,Ute Lisenfeld,Florent Renaud +9 more
TL;DR: In this article , the authors report atomic hydrogen (H i ) observations in the vicinity of the Stephan's Quintet (SQ) with a smoothed sensitivity of 1 σ = 4.2 × 10 16 cm −2 per channel (velocity bin-width Δ v = 20 km s −1 ; angular resolution = 4′), which are about two orders of magnitude deeper than previous observations.
Catching Quenching Galaxies: The Nature of the WISE Infrared Transition Zone
Katherine Alatalo,Sabrina Cales,Sabrina Cales,Philip N. Appleton,Lisa J. Kewley,Mark Lacy,Ute Lisenfeld,Kristina Nyland,Jeffrey A. Rich,Jeffrey A. Rich +9 more
TL;DR: In this paper, a prominent bifurcation between early-type and late-type galaxies was found in [4.6]-[12] micron colors from the Wide Field Infrared Survey Explorer (WISE).