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Wide M-dwarf Binaries
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Title: The High-Order-Multiplicity of Unusually Wide M-dwarf Binaries: Eleven New Triple and Quadruple Systems Authors: Nicholas M. Law, Saurav Dhital, Adam L. Kraus, Keivan G. Stassun, Andrew A. West M-dwarfs in extremely wide binary systems are very rare, and may thus have different formati...
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Planetary nebula Tc 1
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NASA Telescope Finds Elusive Buckyballs in Space for First Time Astronomers using NASA's Spitzer Space Telescope have discovered carbon molecules, known as "buckyballs," in space for the first time. Buckyballs are soccer-ball-shaped molecules that were first observed in a labora...
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R136a1
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Astronomers detect 'monster star' They are among the true monsters of space - colossal stars whose size and brightness go well beyond what many scientists thought was even possible. One of the objects, known simply as R136a1, is the most massive ever found. Viewed today, the star has a mass about 265...
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1E 1207.4-5209
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Title: HST and VLT observations of the neutron star 1E 1207.4-5209 Authors: A. De Luca, R.P. Mignani, A. Sartori, W. Hummel, P.A. Caraveo, S. Mereghetti, G.F. Bignami 1E 1207.4-5209, the peculiar Central Compact object in the G296.5+10.0 supernova remnant, has been proposed to be an "anti-...
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HD 36402
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Title: Heated dust around the LMC Wolf-Rayet system HD 36402 (BAT99-38) Authors: P. M. Williams (Institute for Astronomy, Royal Observatory Edinburgh) Infrared photometry of the probable triple WC4 (+O?) +O8I: system HD 36402 (BAT99-38) in the LMC shows emission characteristic of heated dust...
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Solitary Stars
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Single star count ups odds of ET Solitary suns like ours are not as rare as we once thought, boosting the likelihood that there are other life-friendly solar systems in the universe. It is not always easy to tell if a star has a companion, since they are often too close together to distinguish as separat...
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U Pisces
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Maxima of long period variable U Pisces on the 16th July, 2010. Magnitude: 11.0-14.4 Type: Mira Position (2000): RA 01 22 58.48, Dec +12 52 04.0
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S Ceti
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Maxima of long period variable S Ceti on the 15th July, 2010. Magnitude: 8.2-14.2 Type: Mira Position (2000): RA 00 24 03.532, Dec 00 24 03.532
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