Pulsar Astrometry
نویسندگان
چکیده
منابع مشابه
Pulsar Astrometry with the VLBA
Many features of the Very Long Baseline Array (VLBA) contrive to make it the best telescope for pulsar astrometry. The measured proper motions and parallaxes allow distances and transverse velocities to be determined. These in turn provide clues to questions spanning nuclear astrophysics on scales of 10−23 m to the distribution of gas in the Galaxy on scales of 10 m. Three pulsars are discussed...
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This thesis describes the development of DiFX, the first general–purpose software correlator for radio interferometry, and its use with the Australian Long Baseline Array to complete the largest Very Long Baseline Interferometry (VLBI) pulsar astrometry program undertaken to date in the Southern Hemisphere. This two year astrometry program has resulted in the measurement of seven new pulsar par...
متن کاملThe Vela pulsar (PSR B0833-45) proper motion revisited with HST astrometry
Using all the HST WFC/WFPC2 images of the field collected so far, we have performed an accurate relative astrometry analysis to re-assess the value of the Vela pulsar proper motion. Although covering a much shorter time span, our measurement clearly confirms the previous result obtained by Nasuti et al. (1997) using ground-based optical data and nails down the proper motion value to μ = 52 ± 3 ...
متن کاملPrecision southern hemisphere VLBI pulsar astrometry II: measurement of seven parallaxes
Accurate measurement of pulsar distances via astrometry using very long baseline interferometry enables the improvement of Galactic electron density distribution models, improving distance estimates for the vast majority of pulsars for which parallax measurements are unavailable. However, pulsars at southern declinations have been under–represented in previous interferometric astrometry campaig...
متن کاملThe Pulsar-white Dwarf-planet System in Messier 4: Improved Astrometry
A young and undermassive white dwarf has been identified as the possible companion to the millisecond pulsar PSR B1620-26 in Messier 4. This association is important as it then helps constrain the mass of the third body in the system to be of order a few times that of Jupiter. The presence of this planet in M4 has critical implications for planetary formation mechanisms in metal-poor environmen...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1984
ISSN: 0074-1809
DOI: 10.1017/s0074180900078451