XMM-Newton Large Programme Details



PROPOSAL OVERVIEW
Proposal Title Velocity dispersion of the ICM in 3 Disturbed X-ray luminous cool core clusters
Proposal Category Galaxies, Groups of Galaxies, Clusters of Galaxies and Superclusters
Proposal Type LARGE PROGRAM
Proposal Id 084058
Number of Observations 6
Total exposure time (ks) 720

PI DETAILS
PI Prof Andrew Fabian
Institute Institute of Astronomy
Country UNITED KINGDOM

CO-INVESTIGATORS
Name Country
C. Pinto UNITED KINGDOM
H. Russell UNITED KINGDOM
J. Sanders GERMANY
H. Liu UNITED KINGDOM
B. McNamara CANADA

ABSTRACT
We propose to observe 3 X-ray luminous clusters which each have over 10^10 Msun of cold molecular gas in their X-ray cool cores. The ALMA velocity and morphology data indicate that the cold gas is disturbed in these object. If, as Hitomi has shown in the Perseus cluster, the cold gas and ICM share the same velocity field, then we shall measure velocity broadening of the soft X-ray emission lines with the XMM RGS. We shall also measure or constrain mass cooling rates of the ICM below 1-2 keV.

PAPERS
Authors marked in red are (co-)investigators in the proposal

Classification of papers are:
- CLASS 1:   papers that present specific XMM-Newton observations
- CLASS 2: papers that refer to published XMM-Newton results with complementary observations, follow-up analysis, or theoretical analysis
- CLASS 3: further deliveries which resulted from the program and which are made available to the community (e.g. source catalogues, processed images or spectra in public data base)
- CLASS 4: comments and suggestions from PI

CLASS 1 (5 references)
  1. " Suppressed cooling and turbulent heating in the core of X-ray luminous clusters RXCJ1504.1-0248 and Abell 1664 "
    Liu, Haonan; Fabian, Andrew C.; Pinto, Ciro; Russell, Helen R.; Sanders, Jeremy S.; McNamara, Brian R.;
    2021 - Monthly Notices of the Royal Astronomical Society, Volume 505, Issue 2, pp.1589-1599
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2021MNRAS.505.1589L
    DOI: 10.1093/mnras/stab1372

  2. " 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; Bregman, Joel N.; Liu, Jifeng;
    2024 - The Astrophysical Journal Supplement Series, Volume 271, Issue 2, id.62, 18 pp.
    Number of Citations: 1
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024ApJS..271...62P
    DOI: 10.1093/mnras/stad3885

  3. " From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources "
    Rodriguez, Antonio C.;
    2024 - Publications of the Astronomical Society of the Pacific, Volume 136, Issue 5, id.054201, 17 pp.
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024PASP..136e4201R
    DOI: 10.1088/1538-3873/ad357c

  4. " Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE "
    Ma, Xiangyao; Zhang, Yanxia; Zhang, Jingyi; Li, Changhua; Kang, Zihan; Li, Ji;
    2024 - The Astronomical Journal, Volume 168, Issue 5, id.210, 10 pp.
    Number of Citations: 0
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024AJ....168..210M
    DOI: 10.3847/1538-4357/ad6e81

  5. " Hidden cooling flows - IV. More details on Centaurus and the efficiency of AGN feedback in clusters "
    Fabian, A. C.; Ferland, G. J.; Sanders, J. S.; Russell, H. R.; McNamara, B. R.; Pinto, C.; Hlavacek-Larrondo, J.; Walker, S. A.; Ivey, L. R.; McDonald, M.;
    2024 - Monthly Notices of the Royal Astronomical Society, Volume 535, Issue 3, pp.2173-2188
    Number of Citations: 1
    https://ui.adsabs.harvard.edu/search/q=bibcode:2024MNRAS.535.2173F
    DOI: 10.1093/mnras/stae2373