Red Supersiants (RSGs)
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comparing observations and theories of RSG. (from Massey et al., 2008arXiv0801.1806M)
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A review of post-RSG (from Oudmaijer et al., 2008arXiv0801.2315O)
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A review of mass loss from hot massive stars
(from Puls et al., 2008A&ARv..16..209P)
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Atmospheric dynamics of RSG
and interferometric observation of it. (from Chiavassa et al., 2008arXiv0802.1403C)
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A 3D pure LTE radiative transfer code to
derived observables of RSGs. (from Chiavassa, 2008arXiv0802.1399C)
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Bipolar nebular around RSGs
could be shaped by bipolar jets instead of wind interaction. (from Smith, 2008arXiv0802.1746S)
- A cluster of massive RSGs are found near the end of the Galactic Bar. (from Alexander et al., 2009AJ....137.4824A)
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Typical objects
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alpha Ori -- an M2 Iab type
supergiant
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mu Cep -- an RSG showing roughly spherical CSE with asymmetric pattern
inside (from de Wit et al., 2008ApJ...685L..75D)
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NML Cyg -- a red hypergiant
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VX Sgr
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VY CMa
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IRC -10414 (IRAS 18204-1344, OH 17.55 -0.13, RAFGL 2139)
-- A RSG with L*=9x10^4Lsun at a distance of D=2-3kpc, found to harbor
bipolar outflows traced by H2O masers (from Maeda et al., 2008PASJ...60.1057M)
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