Patricia Luppe

Patricia Luppe
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Patricia verified their affiliation via an institutional email.
Verified
Patricia verified their affiliation via an institutional email.
  • Master of Science
  • PostDoc Position at Trinity College Dublin

About

5
Publications
192
Reads
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47
Citations
Introduction
Patricia Luppe currently works at the Astrophysical Institute and University Observatory , Friedrich Schiller University Jena. Patricia does research in Theoretical Physics.
Current institution
Trinity College Dublin
Current position
  • PostDoc Position
Additional affiliations
June 2017 - present
Friedrich Schiller University Jena
Position
  • PhD Student
June 2017 - present
Friedrich Schiller University Jena
Position
  • PhD Student

Publications

Publications (5)
Article
As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas and dust in Giant Molecular Clouds (GMCs), how it moves, how it is affected by the nearby massive stars, and which portions of those GMCs eventually collapse into star f...
Preprint
Full-text available
Submillimeter and millimeter wavelengths provide a unique view of the Universe, from the gas and dust that fills and surrounds galaxies to the chromosphere of our own Sun. Current single-dish facilities have presented a tantalising view of the brightest (sub-)mm sources, and interferometers have provided the exquisite resolution necessary to analys...
Article
As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas and dust in Giant Molecular Clouds (GMCs), how it moves, how it is affected by the nearby massive stars, and which portions of those GMCs eventually collapse into star f...
Article
Full-text available
Debris discs are second generation dusty discs formed by collisions of planetesimals. Many debris discs have been found and resolved around hot and solar-type stars. However, only a handful have been discovered around M-stars, and the reasons for their paucity remain unclear. Here we check whether the sensitivity and wavelength coverage of present-...
Preprint
Debris discs are second generation dusty discs formed by collisions of planetesimals. Many debris discs have been found and resolved around hot and solar-type stars. However, only a handful have been discovered around M-stars, and the reasons for their paucity remain unclear. Here we check whether the sensitivity and wavelength coverage of present-...

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