| Name | 086125 |
| Title | Elemental abundances of LIRG Arp299 |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0861250101 |
| DOI | https://doi.org/esa-[xxxxxxx] |
| Author | Dr Junjie Mao |
| Description | Specific abundance patterns are left by distinct chemical enrichment processes during the formation and evolution of galaxies. We propose to observe the luminous infrared galaxy Arp 299 with a total exposure of 130 ks. The existing RGS spectrum with a short exposure yields rather high Mg-O and Ne-O abundance ratios (with large uncertainties) in the hot atmosphere of the host galaxy. Core-collapse supernovae are the main metal factory of these elements. Nonetheless, the observed abundance ratios are in tension with various initial mass function weighted yields at the 1-2 sigma confidence level. Combining the archival and proposed observations, we can accurately measure the metal abundances. We will explore possible origins of the unusual abundance ratios. |
| Publication | No observations found associated with the current proposal |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2020-05-08T20:18:02Z/2020-11-23T00:35:03Z |
| 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 | 2021-12-15T00:00:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2021-12-15T00:00:00Z, 086125, 18.02_20200221_1200. https://doi.org/esa-[xxxxxxx] |