The CMa R1 region includes the arc-shaped ionized nebula S2-296, suggested to bean old supernova remnant, as well as several very young (less than 5 Myr)clusters. Based on archival ROSAT observations covering nearly 5 sq. deg. wehave discovered a new, 10Myr old cluster that may be a fossil from a distinct,past star-formation episode, suggesting sequential star formation betweensupernova cavities. We propose a mosaic of 5 x 30ks EPIC fields to reveal amixed population from both older and young clusters corresponding respectivelyto a fossil, and to an onging, star formation episode.
Star formation history of Canis Major OB1. II. A bimodal X-ray population revealed by XMM-Newton |Santos-Silva, T., Gregorio-Hetem, J., et al. | A&A | 609-127 | 2018 | 2018A&A...609A.127S | http://ui.adsabs.harvard.edu/#abs/2018A&A...609A.127S
Searching for Active Low-mass Stars in the CMa Star-forming Region: Multi-band Photometry with T80S |Gregorio-Hetem, J., Navarete, F., et al. | AJ | 161-133 | 2021 | 2021AJ....161..133G | http://ui.adsabs.harvard.edu/#abs/2021AJ....161..133G
Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earth.s Magnetosphere to the Solar Wind Proton Flux |Zhang, Yingjie, Sun, Tianran, et al. | ApJ | 948-69 | 2023 | 2023ApJ...948...69Z | http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z
Robust constraints on feebly interacting particles using XMM-Newton |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-L101305 | 2024 | 2024PhRvD.109j1305L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L
Multimessenger search for electrophilic feebly interacting particles from supernovae |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-103028 | 2024 | 2024PhRvD.109j3028L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L
Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints |De la Torre Luque, Pedro, Balaji, Shyam, | ApJ | 968-46 | 2024 | 2024ApJ...968...46D | http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2010-10-25T13:26:04Z/2011-04-11T22:10:19Z
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.
European Space Agency, Prof Jane Gregorio-Hetem, 2012, 'Fossil sequential star formation in the CMa R1 regionquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-a0zqdgo
