87 citations · 381 across the 15 of their papers we have counts for
7 papers · 2 filters
Does tiny-scale atomic structure exist in the interstellar medium ?
S. Stanimirovic, J. M. Weisberg, A. Hedden +4
We report on preliminary results from the recent multi-epoch neutral hydrogen absorption measurements toward three pulsars, B0823+26, B1133+16 and B2016+28, using the Arecibo teles…
A Low Frequency Survey of the Galactic Plane Near l=11 degrees: Discovery of Three New Supernova Remnants
C. L. Brogan, K. E. Devine, T. J. Lazio +5
We have imaged a 1 deg^2 field centered on the known Galactic supernova remnant (SNR) G11.2-0.3 at 74, 330, and 1465 MHz with the Very Large Array radio telescope (VLA) and 235 MHz…
Arecibo 430 MHz Pulsar Polarimetry: Faraday Rotation Measures and Morphological Classifications
J. M. Weisberg, J. M. Cordes, B. Kuan +3
We have measured Faraday Rotation Measures (RMs) at Arecibo Observatory for 36 pulsars, 17 of them new. We combine these and earlier measurements to study the galactic magnetic fie…
Phase-Referenced VLBA Observations of OH Masers at 4765 MHz
Patrick Palmer, W. M. Goss, K. E. Devine
We report VLBA observations of maser emission from the rotationally excited doublet Pi 1/2, J=1/2 state of OH at 4765 MHz. We made phase-referenced observations of W3(OH) at both 4…
The tiny-scale atomic structure: gas cloudlets or scintillation phenomenon ?
S. Stanimirovic, J. M. Weisberg, A. Hedden +3
We present preliminary results from the recent multi-epoch HI absorption measurements toward several pulsars using the Arecibo telescope. We do not find significant variations in o…
PSR B1849+00 probes the tiny-scale molecular gas?
S. Stanimirovic, J. M. Weisberg, J. M. Dickey +4
In this paper we present and discuss the great difference in OH absorption spectra against PSR B1849+00 and SNR G33.6+0.1 along the same line-of-sight. This finding is important as…