Results 121 to 130 of about 12,394 (217)
The Astronomical Journal, 1981 Approximately 70 M supergiants have been searched for Type I OH emission. OH was detected toward six stars but it is probably not associated with the stars in most cases. The results of this survey, combined with earlier searches for Type II OH supergiants, indicate that the OH luminosities are less for Type I supergiants than for Type II supergiants ...
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A Model for Eruptive Mass Loss in Massive Stars
The Astrophysical JournalEruptive mass loss in massive stars is known to occur, but the mechanism(s) are not yet well understood. One proposed physical explanation appeals to opacity-driven super-Eddington luminosities in stellar envelopes.
Shelley J. Cheng +5 more
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The Astrophysical Journal Supplement SeriesTo study how massive variable stars affect their environment, we search for variability among Zwicky Transient Facility (ZTF) sources located within the optical extent of the nearby starburst galaxy IC 10.
Zehao Jin, Joseph D. Gelfand
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The evolution of massive stars: bridging the gap in the Local Group. [PDF]
Philos Trans A Math Phys Eng Sci, 2017 Massey P, Neugent KF, Levesque EM.
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Bridging the gap: from massive stars to supernovae. [PDF]
Philos Trans A Math Phys Eng Sci, 2017 Maund JR +3 more
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Description of the supergiant isopod Bathynomus raksasa sp. nov. (Crustacea, Isopoda, Cirolanidae) from southern Java, the first record of the genus from Indonesia. [PDF]
Zookeys, 2020 Sidabalok CM, Wong HP, Ng PKL.
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<i>Bathynomus vaderi</i> Ng, Sidabalok & Nguyen, 2025: the senior synonym of <i>B. paracelensis</i> Huang & Kawai, 2025 (Crustacea, Isopoda, Cirolanidae). [PDF]
ZookeysNg PKL +5 more
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Information-Entropy Analysis of Stellar Evolutionary Stages with Application to FS CMa Objects. [PDF]
Entropy (Basel)Zhanabaev Z, Akniyazova A, Ashimov Y.
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