Evidence for massive warm-hot circumgalactic medium around NGC 3221
Sanskriti Das, Smita Mathur, Anjali Gupta, Fabrizio Nicastro, Yair, Krongold, Cody Null

TL;DR
This study presents the first detection of an extensive warm-hot circumgalactic medium around NGC 3221, revealing its mass, extent, and contribution to the galaxy's baryon budget, consistent with cosmological expectations.
Contribution
It provides the first observational evidence of a massive warm-hot CGM around an external L* star-forming spiral galaxy, using deep Suzaku X-ray observations.
Findings
Detected the warm-hot CGM at 3.4σ significance.
Estimated the gas mass to be approximately 16 billion solar masses.
Found the baryon fraction consistent with cosmological values.
Abstract
We report a 3.4 detection of the warm-hot, massive, extended circumgalactic medium (CGM) around an L star-forming spiral galaxy NGC 3221, using deep Suzaku observations. The temperature of the gas is K, comparable to that of the Milky Way CGM. The spatial extent of the gas is at least kpc. For a -model of density profile with solar abundance, the central emission measure is EM = cm kpc and the central electron density is cm, with a slope of . We investigate a range of values, and find that the details of the density profile do not change our results significantly. The mass of the warm-hot gas, assuming a metallicity of Z is M, being the most massive baryon component of NGC 3221. The baryon fraction is…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
