A dataset provided by the European Space Agency

Name 067474
Title Do hybrid morphology radio sources form in a lopsided distribution of cold gas?
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674740101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674740201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674740301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674740401

DOI https://doi.org/10.5270/esa-npqabch
Author Dr Brendan Miller
Description We test the hypothesis that hybrid morphology radio sources (HYMORS; Gopal-Krishna & Wiita 2000) feature one-sided jet disruption caused by propagation into a large-scale overdensity of cold gas, through XMM-Newton observations of B2 1404+25A and B2 1345+28 (33 and 16 ks, respectively). These HYMORS are intrinsic low-inclination RLQs for which the X-ray spectra would ordinarily be unabsorbed. VLBA mapping places the FRI jet on the near side in B2 1404+25A, and so the putative disrupting medium can be directly detected as absorption against the core; in contrast, the FRII lobe is closer in B2 1345+28, and so a simple power-law X-ray spectrum is anticipated. Distinct results are predicted for alternative scenarios of HYMORS formation.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-12-13T15:35:12Z/2011-12-18T04:41:44Z
Version 17.56_20190403_1200
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 2013-01-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-01-20T00:00:00Z, 067474, 17.56_20190403_1200. https://doi.org/10.5270/esa-npqabch