(When) Are Filaments Fundamental?
<|begin_of_text|><|start_header_id|>system<|end_header_id|> You are a research archivist expert in dataset metadata. Answer the question truthfully.  <|eot_id|><|start_header_id|>user<|end_header_id|> Here is the Description of a dataset. Description:'Presentation Date: Monday, April 3, 2017.Location: Department Seminar, Department of Astrophysics, University of Vienna. Abstract: As the resolution of imaging of the dense interstellar medium has improved, we have gone from a very blobby view, featuring interstellar “clouds' to a much more “stringy' view, featuring interstellar “filaments.” Some three-dimensional shapes in the ISM have a very limited set of possible origins: for example, disks essentially require rotation to be generated. But, prominent filaments (or at least the appearance thereof) can be created by a variety of processes, including various combinations of turbulence, shocks, and fragmentation—all of which can be driven by combinations of gravitational, magnetic and thermal forces. In this talk, I will focus primarily on two kinds of filaments, on two very diffe' . Please return only a json list of at most 3 Keywords corresponding to the Description:.<|eot_id|><|start_header_id|>assistant<|end_header_id|> {"Answer" : ["filaments"]} <|eot_id|>
 Here is the Description of a dataset. Description:'Presentation Date: Monday, April 3, 2017.Location: Department Seminar, Department of Astrophysics, University of Vienna. Abstract: As the resolution of imaging of the dense interstellar medium has improved, we have gone from a very blobby view, featuring interstellar “clouds' to a much more “stringy' view, featuring interstellar “filaments.” Some three-dimensional shapes in the ISM have a very limited set of possible origins: for example, disks essentially require rotation to be generated. But, prominent filaments (or at least the appearance thereof) can be created by a variety of processes, including various combinations of turbulence, shocks, and fragmentation—all of which can be driven by combinations of gravitational, magnetic and thermal forces. In this talk, I will focus primarily on two kinds of filaments, on two very diffe' . Please return only a json list of at most 3 Keywords corresponding to the Description:.
Presentation Date: Monday, April 3, 2017.Location: Department Seminar, Department of Astrophysics, University of Vienna. Abstract: As the resolution of imaging of the dense interstellar medium has improved, we have gone from a very blobby view, featuring interstellar “clouds' to a much more “stringy' view, featuring interstellar “filaments.” Some three-dimensional shapes in the ISM have a very limited set of possible origins: for example, disks essentially require rotation to be generated. But, prominent filaments (or at least the appearance thereof) can be created by a variety of processes, including various combinations of turbulence, shocks, and fragmentation—all of which can be driven by combinations of gravitational, magnetic and thermal forces. In this talk, I will focus primarily on two kinds of filaments, on two very diffe
filaments