Zobrazeno 1 - 10
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pro vyhledávání: '"Ranasinghe, S."'
Autor:
Ranasinghe, S., Leahy, D.
We present an revised table of 390 Galactic radio supernova remnants (SNRs) and their basic parameters. Statistical analyses are performed on SNR diameters, ages, spectral indices, Galactic heights and spherical symmetries. Furthermore, the accuracy
Externí odkaz:
http://arxiv.org/abs/2302.06593
Autor:
Ranasinghe, S., Leahy, D.
We present a table of 215 SNRs with distances. New distances are found to SNR G$51.26+0.11$ of $6.6 \pm 1.7$ kpc using HI absorption spectra, and to 5 other SNRs using maser/molecular cloud associations. We recalculate the distances and errors to all
Externí odkaz:
http://arxiv.org/abs/2209.04570
Publikováno v:
Universe 2021, 7(9), 338
Young Supernova remnants (SNRs) with smaller angular sizes are likely missing from existing radio SNR catalogues, caused by observational constraints and selection effects. In order to find new compact radio SNR candidates, we searched the high angul
Externí odkaz:
http://arxiv.org/abs/2109.07003
Publikováno v:
Journal of High Energy Physics, Gravitation and Cosmology. 6(2020) 9-19
HI spectra of the supernova remnant G18.9-1.1 and the supernova remnant candidate G28.6+0.0 are analyzed. We compared the spectra to $^{13}$CO emission spectra and to spectra of HII regions in the area to determine kinematic distances. G18.9-1.1 is a
Externí odkaz:
http://arxiv.org/abs/1910.05407
Autor:
Rathnayaka, A. M. A. I., Perera, W. N. D., Savindu, H. P., Madarasingha, K. C. M., Ranasinghe, S. P., Thuduwage, H. G. T. V., Kulathilaka, A. U., Silva, P., Jayasinghe, S., Kahaduwa, K. T. D., De Silva, A. C.
Foot plantar pressure monitoring is an important tool for biomechanical assessment of posture, foot complications due to callus formation and wounds and for sports applications. The pronounced cost associated with commercial plantar pressure monitori
Externí odkaz:
http://arxiv.org/abs/1901.05303
Autor:
Ranasinghe, S., Leahy, D. A.
We carry out a comprehensive study of HI 21 cm line observations and $^{13}$CO line observations of 21 supernova remnants (SNRs). The aim of the study is to search for HI absorption features to obtain kinematic distances in a consistent manner. The 2
Externí odkaz:
http://arxiv.org/abs/1808.09082
Autor:
Leahy, D. A., Ranasinghe, S.
Recent studies using 21 cm HI line and $^{13}$CO line observations in the inner part of the Galaxy have resulted in new distances for 30 Galactic supernova remnants (SNRs). 15 of those remnants have observed X-ray spectra, for which shocked-gas tempe
Externí odkaz:
http://arxiv.org/abs/1808.04716
Autor:
Ranasinghe, S., Leahy, D. A.
Accurate distances to supernova remnants (SNRs) are crucial in determining their size, age, luminosity and evolutionary state. To determine distances, we chose three SNRs from the VLA Galactic Plane Survey (VGPS) for extraction of HI absorption spect
Externí odkaz:
http://arxiv.org/abs/1712.04423
Distances are found for four supernova remnants without previous distance measurements. H I spectra and H I channel maps are used to determine the maximum velocity of H I absorption for the four supernova remnants (SNRs). We examined $^{13}$CO emissi
Externí odkaz:
http://arxiv.org/abs/1712.04515
Autor:
Sundelin, M.O., Silva, J.D.C., Daele, A.V., Savopoulos, V., Pirola, G.M., Ranasinghe, S., Cleynenbreugel, B.V., Biyani, C.S. *, Kailavasan, M.
Publikováno v:
In Actas Urológicas Españolas (English Edition) January-February 2021 45(1):49-56