A dataset provided by the European Space Agency

Name: Winding the Spiral: XMM Observations of the Spiral Planetary Nebula
Published: 2019-02-15T23:00:00Z

Proposal ID	080196
Title	Winding the Spiral: XMM Observations of the Spiral Planetary Nebula
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0801960101
DOI	https://doi.org/10.5270/esa-7mgsssx
Principal Investigator, PI	Dr Rodolfo Montez
Abstract	The Spiral Planetary Nebula (NGC 5189), exhibits spectacular point-symmetricmorphology indicative of a number of collimated outflows. The WO1 central starhas lost its hydrogen-rich envelope, possibly through a late thermal pulse orbinary interaction. The recent discovery of a compact companion to the WO1central star in 4 day orbit connects the morphological properties of the nebulawith powerful binary interactions, potentially as a result of post-commonenvelope binary evolution. Several processes may be responsible for X-rayemission originating from NGC 5189, including a hot bubble, wind shocks, andcompanion activity. Our requested 80 ks XMM observation will be the firstpointed X-ray observation of this exotic PN.
Publications	A Carbon-rich Hot Bubble in the Planetary Nebula NGC 5189 \|Toalu00e1 Jesu00fas A. Montez Rodolfo Jr. \| ApJ \| 886-30 \| 2019 \| 2019ApJ...886...30T \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...886...30T X-ray Observations of Planetary Nebulae since WORKPLANS I and Beyond \|Guerrero Martu00edn A. \| Galax \| 8-24 \| 2020 \| 2020Galax...8...24G \| http://ui.adsabs.harvard.edu/#abs/2020Galax...8...24G Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-02-05T07:00:48Z/2018-02-06T07:25:53Z
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	2019-02-15T23:00:00Z
Last Update	2025-01-27
Keywords	"central star", "NGC 5189", "compact companion", "symmetric morphology indicative", "companion activity", "xray emission", "orbit connects", "wind shoc", "powerful binary interactions", "exotic pn", "hydrogen rich envelope", "binary interaction", "spiral planetary nebula", "collimated outflows", "ngc 5189", "morphological properties", "hot bubble", "envelope binary evolution", "late thermal pulse", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Rodolfo Montez, 2019, 'Winding the Spiral: XMM Observations of the Spiral Planetary Nebula', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7mgsssx