On the Ionizing Sources in Spiral Galaxies: I. From Central Regions to Thick Disk and Disk-Halo Connection

Simple item page
dc.creatorSamurovic, S.
dc.creatorCirkovic, M. M.
dc.creatorMilosevic-Zdjelar, V.
dc.creatorPetrovic, J.
dc.date1998-08-07
dc.date.accessioned2026-07-07T02:27:34Z
dc.date.available2026-07-07T02:27:34Z
dc.descriptionWe study the ionizing sources in spiral galaxies and examine in more detail our Galaxy. Using Taylor & Cordes (1993) model we analyze the electron density in different parts of the Galaxy, and emphasize the still unsolved problems. Finally, we compare the intensities of H$α$ emission in disk and halo.
dc.description5 pages, plain TeX, 1 figure, uses psfig, accepted as a contribution to the 19th Summer School and International Symposium of the Physics of Ionized Gases (SPIG), to be held at Zlatibor, Yugoslavia, August 31-September 4, 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9808063
dc.identifierhttp://arxiv.org/abs/astro-ph/9808063
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12748
dc.subjectAstrophysics
dc.titleOn the Ionizing Sources in Spiral Galaxies: I. From Central Regions to Thick Disk and Disk-Halo Connection
dc.typetext

Files

Collections

arXiv