106 citations · 499 across the 11 of their papers we have counts for
11 papers
The Mass Evolution of Protostellar Disks and Envelopes in the Perseus Molecular Cloud
Bridget C. Andersen, Ian W. Stephens, Michael M. Dunham +8
In the standard picture for low-mass star formation, a dense molecular cloud undergoes gravitational collapse to form a protostellar system consisting of a new central star, a circ…
Chemistry of a newly detected circumbinary disk in Ophiuchus
E. Artur de la Villarmois, L. E. Kristensen, J. K. Jørgensen +6
(Abridged) Astronomers recently started discovering exoplanets around binary systems. Therefore, understanding the formation and evolution of circumbinary disks is crucial for a co…
Episodic accretion: the interplay of infall and disc instabilities
Michael Kuffmeier, Søren Frimann, Sigurd S. Jensen +1
Using zoom-simulations carried out with the adaptive mesh-refinement code RAMSES with a dynamic range of up to we investigate the accretion profil…
Supernova Driving. IV. The Star Formation Rate of Molecular Clouds
Paolo Padoan, Troels Haugbølle, Åke Nordlund +1
We compute the star formation rate (SFR) in molecular clouds (MCs) that originate {\it ab initio} in a new, higher-resolution simulation of supernova-driven turbulence. Because of…
Protostellar accretion traced with chemistry. High resolution C18O and continuum observations towards deeply embedded protostars in Perseus
Søren Frimann, Jes K. Jørgensen, Michael M. Dunham +6
Context: Understanding how accretion proceeds is a key question of star formation, with important implications for both the physical and chemical evolution of young stellar objects…
The Astropy Problem
Demitri Muna, Michael Alexander, Alice Allen +151
The Astropy Project (http://astropy.org) is, in its own words, "a community effort to develop a single core package for Astronomy in Python and foster interoperability between Pyth…
Water around IRAS15398-3359 observed with ALMA
P. Bjerkeli, J. K. Jørgensen, E. A. Bergin +9
How protostars accrete mass is one of the fundamental problems of star formation. High column densities and complex kinematical structures make direct observations challenging and…
Protostellar accretion traced with chemistry: Comparing synthetic C18O maps of embedded protostars to real observations
Søren Frimann, Jes K. Jørgensen, Paolo Padoan +1
Context: Understanding how protostars accrete their mass is a central question of star formation. One aspect of this is trying to understand whether the time evolution of accretion…
Large-scale numerical simulations of star formation put to the test: Comparing synthetic images and actual observations for statistical samples of protostars
Søren Frimann, Jes K. Jørgensen, Troels Haugbølle
(abridged) Context: Both observations and simulations of embedded protostars have progressed rapidly in recent years. Bringing them together is an important step in advancing our k…
Sounding stellar cycles with Kepler - II. Ground-based observations
C. Karoff, T. S. Metcalfe, W. J. Chaplin +11
We have monitored 20 Sun-like stars in the Kepler field-of-view for excess flux with the FIES spectrograph on the Nordic Optical Telescope since the launch of Kepler spacecraft in…
The first evidence for multiple pulsation axes: a new roAp star in the Kepler field, KIC 10195926
D. W. Kurtz, M. S. Cunha, H. Saio +14
We have discovered a new rapidly oscillating Ap star among the Kepler Mission target stars, KIC 10195926. This star shows two pulsation modes with periods that are amongst the long…