The dynamo model of solar magnetic field generation assumes that magnetic flux is retained at the dynamo site for times of the order of the solar-cycle period. However, flux tubes in the solar convection zone are expected to be buoyant, rising to the surface on timescales much shorter than the solar cycle. Since the initial 1955 paper by Parker on

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We present a study of the diffuse ionized gas (DIG) for a sample of nearby spiral galaxies using Hα images, after constructing their H II region catalogues. The integrated Hα emission of the DIG accounts for between 25% to 60% of the total Hα of the galaxy and a high ionizing photon flux is necessary to keep this gas ionized. We suggest that Lyman

Available from the Minor Planet Center.

We present the latest results from the Chandra survey/monitoring program of M31. We will present spectral and timing information on the point sources, including the nuclear source which may be associated with the central supermassive black hole. There are more than 120 point sources (including 18 globular clusters) detected in the central region

The Chandra Multiwavelength Plane (ChaMPlane) Survey is a project to identify a large sample of serendipitous X-ray sources located to arcsec precision in deep (≳ 30 ksec) galactic fields (b ~ 10 degree) imaged by the Chandra X-ray Observatory. Our primary goal is to identify Cataclysmic Variables (CVs) and quiescent Low Mass X-ray Binaries