A dataset provided by the European Space Agency

Name 076289
Title Detailed study of PSR B0656+14
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762890101

DOI https://doi.org/10.5270/esa-qr5gv1a
Author Prof Oleg Kargaltsev
Description We propose XMM-Newton and NuSTAR observations of PSR B0656+14. Its X-ray
spectrum shows complex variability with the pulsar.s rotation phase. Our
re-analysis of archival data suggests that much of the variability could be due
to spectral feature(s) rather than a hot polar cap. If confirmed, it would only
be the second case when such features are seen in the spectrum of a
rotation-powered pulsar. The origin of the features must be intimately linked to
the properties of NS atmospheres or magnetospheres. However, one should study
the features in more than one pulsar before a definitive interpretation can be
given. In addition, our observations will fill in the gap in the multiwavelength
spectrum of B0656+14 by measuring its non-thermal spectrum above 6 keV.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2015-09-19T19:55:22Z/2015-09-21T08:02:02Z
Version 14.21_20150826_1500
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2016-10-05T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Oleg Kargaltsev, 2016, 076289, 14.21_20150826_1500, European Space Agency, https://doi.org/10.5270/esa-qr5gv1a