Proposal ID | 065565 |
Title | Unveiling young Pulsars and their Wind Nebulae through hard X-rays |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655650201 |
DOI | https://doi.org/10.5270/esa-k08sjh7 |
Principal Investigator, PI | Dr Fabio Mattana |
Abstract | The INTEGRAL mission has recently accessed the yet poorly known population ofpulsars and their wind nebulae radiating above 20 keV. However, INTEGRAL hasalso pinpointed several new sources (e.g. IGR J14003-6326, IGR J18135-1751)which follow-up observations proved to be young and X-ray bright pulsars or PWN.We propose a research program aimed at identifying four new persistent hardX-ray unknown sources at low Galactic latitude, selected from the latestINTEGRAL survey as the best candidates for new young pulsar/PWN systems. Theseobjects lack any obvious infrared or optical counterpart, and have never beenobserved in soft X-rays. With short (5 10 ks) XMM-Newton observations, we willable to locate them, characterize their spectrum, and find their possible non-thermal diffuse emission. |
Publications |
|
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2010-10-10T22:11:19Z/2010-10-11T01:28:11Z |
Version | 17.56_20190403_1200 |
Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2011-10-28T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "igr j18135 1751", "persistent hard xray", "hard xray", "wind nebulae", "xmm newton", "integral mission", "low galactic latitude", "XMM-Newton", "xray bright pulsars", "integral survey", "soft xray", "XMM", "wind nebulae radiating", "optical counterpart", "research program aimed", "igr j14003 6326", "pwn systems", "nonthermal diffuse emission" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Fabio Mattana, 2011, 'Unveiling young Pulsars and their Wind Nebulae through hard X-rays', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-k08sjh7 |