A dataset provided by the European Space Agency

Name 072820
Title Fundamental properties of novae outburst
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728200201

DOI https://doi.org/10.5270/esa-jmxt629
Author Dr Gregory Schwarz
Description We propose non-disruptive ToO observations of two optically bright Galactic
novae in outburst to observe their temporal UV evolution using the HST/STIS
echelle. One ToO will target a Carbon-Oxygen type nova and the other ToO will be
reserved for the next high energy gamma-ray detected nova. The Fermi/LAT
detection of high energy gamma-rays is a recent and unexpected discovery whose
mechanism in classical novae is not currently understood. In both cases, UV
spectroscopy is essential for determining elemental abundances, mass, dynamics,
and structure. Each nova target would also be observed with a single, high
resolution XMM/RGS exposure obtained while X-ray luminous (as determined by our
Swift X-ray monitoring).
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-11-21T13:11:10Z/2013-11-21T22:34:50Z
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 2014-12-05T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Gregory Schwarz, 2014, 072820, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jmxt629