Name | 087101 |
Title | UNDERSTANDING THE GAMMA-RAY PRODUCTION MECHANISM IN NOVA SHOCKS |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0871010101 |
DOI | https://doi.org/esa-[xxxxxxx] |
Author | Dr Kirill Sokolovsky |
Description | We propose a 60ks observation for one new GeV bright nova to explore the particle acceleration and gamma-ray production mechanisms. We will constrain the particle acceleration efficiency by comparing thermal X-ray to GeV luminosity and search for predicted non-thermal X-rays. Understanding shocks in novae is r^ant for other shock-powered transients including Type IIn supernovae, tidal disruption events and stellar mergers. NuSTAR is the only instrument capable of detecting X-rays from novae simultaneously with the GeV emission (the lower energy X-rays accessible to other focusing instruments are hidden by the nova shell at these times). The observations should be conducted now to take advantage of the simultaneous operations with Fermi-LAT. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, RGS1, RGS2 |
Temporal Coverage | 2020-09-23T11:05:36Z/2020-09-23T21:22:50Z |
Version | 18.02_20200221_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 | 2021-10-20T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2021-10-20T00:00:00Z, 087101, 18.02_20200221_1200. https://doi.org/esa-[xxxxxxx] |