Abstract |
XMM observations of the bright Cepheids Polaris, delta Cep and beta Dor willsolve two important puzzles recently uncovered in Cepheids with Chandra andFUSE. Recently, with Chandra, we discovered Polaris, a low amplitude ClassicalCepheid, to be a soft, log Lx = 28.8 ergs/sec X-ray source. Archival FUSEspectra of Polaris and beta Dor contain prominent emission lines of C III 977and O VI 1032/1038, indicating hot plasma with temperatures of at least 500,000K. Although Chandra detected Polaris as an X-ray source, the 10-ksec ACIS-Iexposure is inadequate to definitively distinguish between the supergiantPolaris or a mid-F main sequence companion. |
Publications |
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- Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks |Kosiba, Matej, Lieu, Maggie, et al. | MNRAS | 496-4141 | 2020 | 2020MNRAS.496.4141K | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K
- SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release |Clerc, N., Kirkpatrick, C. C., et al. | MNRAS | 497-3976 | 2020 | 2020MNRAS.497.3976C | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C
- An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge |Qu, Zhijie, Huang, Rui, et al. | ApJ | 907-14 | 2021 | 2021ApJ...907...14Q | http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q
- 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
- The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines |Qu, Zhijie, Koutroumpa, Dimitra, et al. | ApJ | 930-21 | 2022 | 2022ApJ...930...21Q | http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q
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- Selection of Compton-thick AGN from a hard photometric sample using XMM-Newton observations |Mostafa, Reham, Guainazzi, Matteo, | MNRAS | 525-5080 | 2023 | 2023MNRAS.525.5080M | http://ui.adsabs.harvard.edu/#abs/2023MNRAS.525.5080M
- The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions |Pan, Zeyang, Qu, Zhijie, et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
- 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
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Keywords |
"vi 1032", "log lx", "delta cep", "XMM", "bright cepheids polaris", "definitively distinguish", "xray source", "sec xray source", "prominent emission lines", "archival fuse spectra", "secret xray lives", "hot plasma", "main sequence companion", "beta dor", "iii 977", "supergiant polaris" |