J/PAZh/42/200   Dispersion measure of Milky Way and MC pulsars  (Zhezher+, 2016)

Probing Milky Way's hot gas halo density distribution using the dispersion measure of pulsars. Zhezher Ya.V., Nugaev E.Ya., Rubtsov G.I. <Pis'ma Astron. Zh. 42, 200 (2016)> =2016PAZh...42..200Z 2016PAZh...42..200Z (SIMBAD/NED BibCode) =2016AstL...42..173Z 2016AstL...42..173Z
ADC_Keywords: Milky Way ; Magellanic Clouds ; Pulsars ; Stars, distances Keywords: missing baryons - hot gas - pulsars - dispersion measure Abstract: A number of recent studies indicates a significant amount of ionized gas in a form of the hot gas halo around the Milky Way. The halo extends over the region of 100 kpc and may be acountable for the missing baryon mass. In this paper we calculate the contribution of the proposed halo to the dispersion measure (DM) of the pulsars. The Navarro, Frenk, and White (NFW), Maller and Bullock (MB), and Feldmann, Hooper, and Gnedin (FHG) density distributions are considered for the gas halo. The data set includes pulsars with the distance known independently from the DM, e.g., pulsars in globular clusters, LMC, SMC and pulsars with known parallax. The results exclude the NFW distribution for the hot gas, while the more realisticMB and FHG models are compatible with the observed dispersion measure. Description: In this paper we analyze pulsars in the MilkyWay, in the Large Magellanic Cloud (LMC) and in the Small Magellanic Cloud (SMC). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 41 62 List of Milky Way pulsars with parallaxes table3.dat 38 20 List of LargeMagellanic Cloud and Small Magellanic Cloud pulsars -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Pulsar name (JHHMM+DDMM) 12- 17 F6.2 deg GLON Galactic longitude 19- 24 F6.2 deg GLAT Galactic latitude 26- 31 F6.3 kpc Dist Distance 33- 41 F9.5 pc/cm3 DM ?=- Dispersion measure -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 18-May-2016
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