Type
Article
Keywords
Galaxy: fundamental parameters, ISM: abundances, ISM: clouds, ISM: structure, pulsars: general, radio lines: ISM
Abstract
We have used the Arecibo telescope to measure the H i absorption spectra of eight pulsars. We show how kinematic distance measurements depend on the values of the Galactic constants R0 and 0, and we select our preferred current values from the literature. We then derive kinematic distances for the low-latitude pulsars in our sample and electron densities along their lines of sight. We combine these measurements with all others in the inner Galactic plane visible from Arecibo to study the electron density in this region.
Language
English
Department(s)
Physics and Astronomy
Journal or Book Title
Astrophysical Journal
Publication Year
2008
Issue Month/Season
February
DOI
10.1086/523345
Publisher
American Astronomical Society
Rights Management
Carleton College does not own the copyright to this work and the work is available through the Carleton College Library following the original publisher policies regarding self-archiving. For more information on the copyright status of this work, refer to the current copyright holder.
RoMEO Color
Green
Preprint Archiving
Yes
Postprint Archiving
Yes
Publisher PDF Archiving
Yes
Contributing Organization
Carleton College
Format
application/pdf
Recommended Citation
Weisberg, J. M., S. Stanimirovic, K. Xilouris, A. Hedden,, A. de la Fuente, S. B. Anderson, and F. A. Jenet., "Arecibo HI absorption measurements of pulsars and the electron density at intermediate longitudes in the first galactic quadrant". Astrophysical Journal, vol. 674, no. 1, 2008. Available at: https://doi.org/10.1086/523345. . [Online]. Accessed via Faculty Work. Physics and Astronomy. Carleton Digital Commons. https://digitalcommons.carleton.edu/phys_faculty/14
The definitive version is available at https://doi.org/10.1086/523345
