Name | 060212 |
Title | A twin cluster to Collinder 69 in the lambda Orionis star forming region |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0602120101 |
DOI | https://doi.org/10.5270/esa-toh4srj |
Author | Dr Beate Stelzer |
Description | The lambda Ori star forming region (5 Myr, 400 pc) is surrounded by a 5 x 5 deg wide molecular ring probably formed by a supernova explosion. Our previous multi-wavelength studies focused on the most well-known areas within the cloud complex. For a complete picture of star formation, believed to be determined by the supernova blast, the large-scale distribution of the pre-main sequence population in lambda Ori needs to be examined. We suspect a further pre-main sequence cluster to be associated with a concentration of B-type stars near the NE of the molecular ring. A search for X-ray emission is the most efficient way of identifying the low-mass cluster. The properties of its members will then be compared to the other lambda Ori subgroups. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2009-09-05T23:06:37Z/2009-09-06T13:32:08Z |
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 | 2010-09-22T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Beate Stelzer, 2010, 060212, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-toh4srj |