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New observations of pulsed X-ray emission from NP 0532

Journal Article · · Astrophysical Journal
DOI:https://doi.org/10.1086/182019· OSTI ID:4036668

Large-area proportional counters sensitive from 0.6 to 23 keV were used to observe about 3 min of pulsed X-ray emission from NP 0532 during two lunar occultation experiments. A detailed pulse profile with 65 $mu$s resolution shows that the x-ray primary pulse shape is essentially identical to its optical counterpart. Spectral data on the pulsed X-ray emission are presented. A pulse- by-pulse examination of the data shows no evidence for temporal variability. (AIP)

Research Organization:
Columbia Astrophysics Laboratory, Columbia University
Sponsoring Organization:
USDOE
NSA Number:
NSA-33-030608
OSTI ID:
4036668
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Vol. 203; ISSN 0004-637X
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English

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