Results 51 to 60 of about 441,928 (76)
MAGELLANIC CLOUDS. XI. SURVEY OF THE NOVAE. [PDF]
Proc Natl Acad Sci U S A, 1954 Henize KG, Hoffleit D, Nail VM.
europepmc +1 more source
Notes on Binary Stars: IV. A Source of Spurious Eccentricity in Spectroscopic Binaries. [PDF]
Proc Natl Acad Sci U S A, 1941 Sterne TE.
europepmc +1 more source
Metadata Guide for STARS [PDF]
, 2016 This Metadata Guide for STARS serves as a guideline in providing metadata for the research and data deposited into STARS, Showcase of Text, Archives, Research & Scholarship, the University of Central Florida\u27s institutional digital repository.
Deng, Sai, Spyers-Duran, Peter
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Herculis Ciofani Sulmonensis in P. Ovidii Nasonis : Libros de Ponto : Observationes
Con: Antiquiss a Nobiliss urbis sulmonis descriptio... con port e pax. propias -- Con: Herculis Ciofani Sulmoniensis in P. Ovisçdii Nasonis Halieuticon... con port. e pax. propias -- Con: Herculis Ciofani Sulmoniensis in P.
Ex offiina Christophoti Plantini +2 more
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, 2015 Workflow outlining the working structure of STARS for projects. The diagram includes responsibilities for Subject Librarians, the Scholarly Communication Librarian, Digital Initiatives, and Metadata/Cataloging.https://stars.library.ucf.edu/stars ...
Dotson, Lee
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Variability of DQ White Dwarfs
White dwarfs are born when a medium to low mass star reaches the end of its evolutionary cycle. A small subset of these stars are the DQ white dwarfs, which have a helium-rich atmosphere and show carbon features. DQs are predicted to have a binary origin,
Adhikari, Paradesh
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Plausible explanations for the variations of orbital period in the old nova DQ Herculis
Astronomy and Astrophysics, 2009 Aims. Several mechanisms are presented to explain the observed small variation in the orbital period of the old nova DQ Herculis. Methods. We have combined two new CCD times of light minimum of DQ Herculis with all 226 available times of light ...
Z. B. Dai, S. B. Qian
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Astrophysical Journal, 1996 We present measurements of cosmic microwave background (CMB) anisotropy near the stars HR 5127 and φ Herculis from the fifth flight of the Millimeter-wave Anisotropy eXperiment (MAX).
Newton Figueiredo
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The nebula around the binary post-AGB star 89 Herculis⋆,⋆⋆
Astronomy and Astrophysics, 2023Iván Gallardo Cava +2 more
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