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M31N 2016-11a
(Preview)
ATel 9768: Liverpool Telescope spectrum of classical nova M31N 2016-11a
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CoRoT 223992193
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Title: CoRoT 223992193: Investigating the variability in a low-mass, pre-main sequence eclipsing binary with evidence of a circumbinary disk Author: Edward Gillen, Suzanne Aigrain, Caroline Terquem, Jerome Bouvier, Silvia H. P. Alencar, Davide Gandolfi, John Stauffer, Ann Marie Cody, Laur...
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Kepler 11145123
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'Roundest known space object' identified Kepler 11145123 is a distant, slowly rotating star that's more than twice the size of the Sun. Researchers were able to show that the difference between its radius as measured to the equator and the radius measured to the poles was just 3km. Read more
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Nova Scorpii 2008
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Title: A low-mass-ratio and deep contact binary as the progenitor of the merger V1309 Sco Author: Li-Ying Zhu, Er-Gang Zhao, Xiao Zhou Nova Sco 2008 (=V1309 Sco) is an example of a V838 Mon type eruption rather than a typical classical nova. This enigmatic object was recently shown to have resulted f...
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SWIFT J175328.5-012704
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ATel 9765: A Deep Radio Limit on the 2016 Decay of Swift J1753.5-0127 from the Very Large Array
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ASASSN-16me
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ATel 9764: Photometric and Spectroscopic Observations of the New Eclipsing Polar ASASSN-16me
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PNV J00424914+4116401
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ATel 9762: Re-brightening of PNV J00424914+4116401
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OGLE16fix
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ATel 9763: VLT Spectroscopic classification of nuclear transient OGLE16fix
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MASTER OT J161532.60+671445.8
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ATel 9760: Fast bright OT in PGC2697102 discovered by MASTER
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MASTER OT J073704.36+250054.5
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ATel 9747: MASTER-Tunka: bright 6mag ampl dwarf nova outburst and OT from MASTER-SAAO
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PNV J09555591+6904050
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ATel 9737: Discovery of a Probable Nova in M81
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AM Canum Venaticorum
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Title: On the Light Curves of AM CVn Author: J. Smak Light curves of AM CVn are analysed by decomposing them into their Fourier components. The amplitudes of the fundamental mode and overtones of the three components: the superhumps, the negative superhumps and the orbital variations, are found to...
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OGLE-2015-BLG-1319
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NASA Space Telescopes Pinpoint Elusive Brown Dwarf Brown dwarfs are thought to be the missing link between planets and stars, with masses up to 80 times that of Jupiter. But their centers are not hot or dense enough to generate energy through nuclear fusion the way stars do. Curiously, scientists ha...
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Swift J0911.9-6452
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ATel 9738: INTEGRAL detection of MAXI J0911-655: still active
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IC 289
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IC 289 (also IC 289, PK 138+02.1, PN G138.8+02.8, IRAS 03062+6107, 2MASS J03101930+6119009) is a magnitude +12.3 planetary nebula located 4200 light-year away in the constellation Cassiopeia. It lies just to the south to the 10th magnitude star TYC 4049-1189-1. The central star is at magnitude +...
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