The Variable Star R Cygni
نویسندگان
چکیده
منابع مشابه
X-ray Emission from the FU Orionis Star V1735 Cygni
The variable star V1735 Cyg (= Elias 1-12) lies in the IC 5146 dark cloud and is a member of the class of FU Orionis objects whose dramatic optical brightenings are thought to be linked to episodic accretion. We report the first X-ray detections of V1735 Cyg and a deeply-embedded class I protostar lying 24 to its northeast. X-ray spectra obtained with EPIC on XMM-Newton reveal very hightemperat...
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[email protected] 2Mizusawa Astrogeodynamics Observatory, National Astronomical Observatory, Mizusawa, Iwate 023-0861 3VERA Project Office, National Astronomical Observatory, Mitaka, Tokyo 181-8588 4Faculty of Science, Kagoshima University, Kagoshima, Kagoshima 890-0065 5Nishi-Harima Astronomical Observatory, Sayo, Hyogo 679-5313 6Nobeyama Radio Observatory, National Astronomical Obs...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1913
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/73.5.390