A zone of avoidance catalogue of 2MASS bright galaxies – I. Sample description and analysis
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This paper describes a new sky survey to be carried out in three wavebands, J(1.25 m), H(1.65 m), and K(2.2 m). The limiting sensitivity of the survey, 10 sigma detection of point sources with K not greater than 14 mag, coupled with its all-sky coverage, were selected primarily to support studies of the large-scale structure of the Milky Way and the Local Universe. The survey requires construction of a pair of observing facilities, one each for the Northern and Southern Hemispheres. Operations are scheduled to begin in 1995. The data will begin becoming publicly available soon thereafter.
To a first approximation, every star is an M dwarf - but there are still considerable gaps in our understanding of these stars, particularly in the space density of the lowest mass stars. Fortunately, the 2 micrometer sky surveys are likely to change this state of affairs. In this paper, I review briefly the likely impact of these surveys.
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The detection of main-sequence circumstellar dust systems provides a powerful tool in the study of possible planetary systems similar to our own.
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We present the discovery of a widely separated (258.3+/-0.4) T dwarf companion to the G1 570ABC system.
We report results of ground-based 10 mu m photometry of main-sequence stars with warm circumstellar dust.
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