R
Roger H. Hildebrand
Researcher at University of Chicago
Publications - 101
Citations - 3519
Roger H. Hildebrand is an academic researcher from University of Chicago. The author has contributed to research in topics: Molecular cloud & Polarimetry. The author has an hindex of 34, co-authored 101 publications receiving 3378 citations. Previous affiliations of Roger H. Hildebrand include ASTRON.
Papers
More filters
Journal ArticleDOI
Far-Infrared Polarimetry of Galactic Clouds from the Kuiper Airborne Observatory
Jessie L. Dotson,Jessie L. Dotson,Jacqueline A. Davidson,C. Darren Dowell,D. A. Schleuning,Roger H. Hildebrand +5 more
TL;DR: In this paper, the authors present a complete summary of the data obtained with the far-infrared polarimeter, Stokes, in flights of the Kuiper Airborne Observatory.
Journal ArticleDOI
Tracing the Magnetic Field in Orion A
Martin Houde,C. Darren Dowell,C. Darren Dowell,Roger H. Hildebrand,Jessie L. Dotson,J. E. Vaillancourt,Thomas G. Phillips,Ruisheng Peng,Pierre Bastien +8 more
TL;DR: In this paper, the orientation of the magnetic field in the plane of the sky relative to the position of the integral-shaped filament in the Orion A star-forming region has been studied.
Journal ArticleDOI
The Shapes and Alignment Properties of Interstellar Dust Grains
Roger H. Hildebrand,M. Dragovan +1 more
Journal ArticleDOI
350 micron Polarimetry from the Caltech Submillimeter Observatory
Jessie L. Dotson,John E. Vaillancourt,L. Kirby,C. Darren Dowell,Roger H. Hildebrand,Jacqueline A. Davidson +5 more
TL;DR: In this article, a summary of data obtained with the 350 micron polarimeter, Hertz, at the Caltech Submillimeter Observatory is presented, along with tabulated results and maps showing polarization vectors and flux contours.
Journal Article
The Determination of Cloud Masses and Dust Characteristics from Submillimetre Thermal Emission
TL;DR: In this paper, the principles by which the dust and masses and total masses of interstellar clouds and certain characteristics of interstellar dust grains can be derived from observations of far infrared and submillimeter thermal emission are reviewed.