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Microquasars are promising candidates to emit high-energy gamma-rays.Moreover, statistical studies show that variable EGRET sources at low galacticlatitudes could be associated with the inner spiral arms. The variable natureand the location in the Galaxy of the high-mass microquasars, concentrated inthe galactic plane and within 55 degrees from the galactic center, give tothese objects the status of likely counterparts of the variable low-latitudeEGRET sources. We consider in this work the two most variable EGRET sources atlow-latitudes: 3EG J1828+0142 and 3EG J1735-1500, proposing a microquasar modelto explain the EGRET data in consistency with the observations at lowerenergies (from radio frequencies to soft gamma-rays) within the EGRET errorbox.Comment: (1)Universitat de Barcelona, (2)Instituto Argentino de  Radioastronomia (3) Facultad de Ciencias Astronomicas y Geofisicas  (4)Lawrence Livermore National Laboratory 6 pages, 2 figures. Presented as a  poster at the V Microquasar Workshop, Beijing, June 2004. Accepted for  publication in the Chinese Journal of Astronomy & Astrophysic

Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500