A new member of the Local Group - The Tucana dwarf galaxy
Russell J. Lavery, Kenneth J. Mighell
Abstract
Russell J. Lavery, Kenneth J. Mighell
Abstract
We present observations of the recently discovered dwarf galaxy in Tucana, which is a likely member of the Local Group. The system is highly flattened and we classify it as dE5. An upper limit on the distance modulus of 24.75 is determined from a V, V- I color-magnitude diagram. This galaxy has a B - R color of 1.1, and with the upper limit to the distance modulus, an absolute R magnitude of - 10. This apparently isolated dwarf system, being on the opposite side of the Milky Way from most of the Local Group, may provide important constraints on Local Group dynamics.
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We present observations of the recently discovered dwarf galaxy in Tucana, which is a likely member of the Local Group. The system is highly flattened and we classify it as dE5. An upper limit on the distance modulus of 24.75 is determined from a V, V- I color-magnitude diagram. This galaxy has a B - R color of 1.1, and with the upper limit to the distance modulus, an absolute R magnitude of - 10. This apparently isolated dwarf system, being on the opposite side of the Milky Way from most of the Local Group, may provide important constraints on Local Group dynamics.
Key concepts: Physics, Local Group, Dwarf galaxy, Dwarf spheroidal galaxy, Astronomy, Galaxy, Astrophysics, Group (periodic table)