کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
8133180 | 1523411 | 2017 | 10 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
The Research on the Profile Stability of the Millisecond Pulsar PSR J1022+1001
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موضوعات مرتبط
مهندسی و علوم پایه
فیزیک و نجوم
نجوم و فیزیک نجومی
پیش نمایش صفحه اول مقاله
چکیده انگلیسی
Pulsars, especially the millisecond pulsars, have very stable integrated pulse profiles. Previous studies found that the integrated pulse profiles of some pulsars exhibit instabilities. In this article, the stability of the integrated pulse profile of millisecond pulsar PSR J1022Â +1001 is investigated. The profile has two peaks, and it is found that the peak ratio significantly changes with time. It is concluded from the analysis that the integrated pulse profile instability of the millisecond pulsar is mainly due to the evolution of the pulse profile with frequency, and in the meanwhile the flux density variations at different frequencies are caused by the interstellar scintillation. It is also found that a small part of integrated pulse profile instability may be due to the intrinsic pulsar properties or other factors.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Chinese Astronomy and Astrophysics - Volume 41, Issue 4, OctoberâDecember 2017, Pages 495-504
Journal: Chinese Astronomy and Astrophysics - Volume 41, Issue 4, OctoberâDecember 2017, Pages 495-504
نویسندگان
Shao Min, You Xiao-peng,