منابع مشابه
SURFACE SCIENCE DAY 11 th December 2017
BOOK Welcome to Surface Science Day @ University of Liverpool 2017! We are pleased to welcome you to the latest in this series of one-day conferences. The inaugural conference was held at the University of Central Lancashire in 2015 and was a great success, though we have even more registrations this time round, with 82 registered participants from 22 different institutes! The event is intended...
متن کاملHigh - resolution radio observations of RCW 49
High-resolution radio continuum observations of the southern H II complex RCW 49 are presented. The observations were carried out with the Molonglo Observatory Synthesis Telescope (MOST) at 0.843 GHz, and the Australia Telescope Compact Array (ATCA) at 1.38 and 2.38 GHz. Two wind-blown shells have been discovered in the core region of RCW 49, the more massive of which surrounds the Westerlund 2...
متن کاملRCW 103 – Revisiting a cooling neutron star
Recent observations of the compact source embedded within the supernova remnant RCW 103 rekindle interest in the origin of this object’s emission. We contrast several models in which neutron-star cooling powers RCW 103. Specifically, either the presence of an accreted envelope or a sufficiently intense magnetic field can account for the X-ray emission from this object. Subject headings: stars: ...
متن کاملNeuroendocrine recovery after 2-week 12-h day and night shifts: an 11-day follow-up.
PURPOSE The study aimed to investigate the course and duration of neuroendocrine recovery after 2-week 12-h day and night shift working periods and to study whether there were differences in recovery between the shift groups. METHODS Twenty-nine male offshore employees working 2-week 12-h shift tours participated in the study; 15 participated after a day shift tour and 14 after a night shift ...
متن کاملPulsar Near the Supernova Remnant RCW 103
Received ; accepted – 2 – ABSTRACT We report the detection of the radio pulsar counterpart to the 69 ms X-ray pulsar discovered near the supernova remnant RCW 103 (G332.4−0.4). Our detection confirms that the pulsations arise from a rotation-powered neutron star, which we name PSR J1617−5055. The observed barycentric period derivative confirms that the pulsar has a characteristic age of only 8 ...
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ژورنال
عنوان ژورنال: The Winnower
سال: 2015
ISSN: 2373-146X
DOI: 10.15200/winn.142802.20776