X-ray Halos around Massive Galaxies: Data and Theory
arXiv:2206.11906 · doi:10.1007/978-981-16-4544-0_110-1
Abstract
The presence of gaseous X-ray halos around massive galaxies is a basic prediction of all past and modern structure formation simulations. The importance of these X-ray halos is further emphasized by the fact that they retain signatures of the physical processes that shape the evolution of galaxies from the highest redshift to the present day. In this review, we overview our current observational and theoretical understanding of hot gaseous X-ray halos around nearby massive galaxies and we also describe the prospects of observing X-ray halos with future instruments.
arXiv commentAccepted chapter of the Section on Galaxies for the Handbook of X-ray and Gamma-ray Astrophysics (Springer, eds. Banbi & Santangelo)
References in corpus (64)
- A Universal Density Profile from Hierarchical Clustering
- Observational Evidence of AGN Feedback
- Heating Hot Atmospheres with Active Galactic Nuclei
- Where are the Baryons?
- The Baryonic Tully-Fisher Relation
- Baryons in the Warm-Hot Intergalactic Medium
- Evolution of Buoyant Bubbles in M87
- Mechanical Feedback from Active Galactic Nuclei in Galaxies, Groups, and Clusters
- Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
- High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies
- The supernova rate per unit mass
- The Baryon Census in a Multiphase Intergalactic Medium: 30% of the Baryons May Still Be Missing
- Testing X-ray Measurements of Galaxy Clusters with Cosmological Simulations
- Where Are the Baryons? II: Feedback Effects
- Low mass X-ray binaries as a stellar mass indicator for the host galaxy
- A high spatial resolution X-ray and H-alpha study of hot gas in the halos of star-forming disk galaxies. I. Spatial and spectral properties of the diffuse X-ray emission
- X-ray source populations in galaxies
- Hot Gas In and Around Elliptical Galaxies
- Stellar and total baryon mass fractions in groups and clusters since redshift 1
- A High Resolution Study of the Hydra A Cluster with Chandra: Comparison of the Core Mass Distribution with Theoretical Predictions and Evidence for Feedback in the Cooling Flow
- A Catalogue and Analysis of X-ray luminosities of Early-type galaxies
- A huge reservoir of ionized gas around the Milky Way: Accounting for the Missing Mass?
- A Chandra View of Dark Matter in Early-Type Galaxies
- Cosmological simulations of the circumgalactic medium with 1 kpc resolution: enhanced HI column densities
- Revisiting with Chandra the Scaling Relations of the X-ray Emission Components (Binaries, Nuclei and Hot Gas) of Early Type Galaxies
- Chandra Observations of NGC 4636 - An Elliptical Galaxy in Turmoil
- Shocks and Cavities from Multiple Outbursts in the Galaxy Group NGC 5813: A Window to AGN Feedback
- Detection of a Hot Gaseous Halo Around the Giant Spiral Galaxy NGC 1961
- X-ray luminosity function of faint point sources in the Milky Way
- X-ray coronae in simulations of disc galaxy formation
- Scaling Mass Profiles around Elliptical Galaxies Observed with Chandra and XMM-Newton
- Galactic winds in the intergalactic medium
- X-ray Scaling Properties of Early-type Galaxies
- A Very Deep Chandra Observation of Abell 2052: Bubbles, Shocks, and Sloshing
- Hot X-ray coronae around massive spiral galaxies: a unique probe of structure formation models
- The MASSIVE Survey IV.: The X-ray halos of the most massive early-type galaxies in the nearby Universe
- Massive Coronae of Galaxies
- XMM-Newton Detects a Hot Gaseous Halo in the Fastest Rotating Spiral Galaxy UGC 12591
- Extended Hot Halos Around Isolated Galaxies Observed in the ROSAT All-Sky Survey
- A Deep XMM-Newton Study of the Hot Gaseous Halo Around NGC 1961
- Diffuse X-Ray Emission from Late-Type Galaxy Haloes
- Hot gas halos around disk galaxies: Confronting cosmological simulations with observations
- X-ray Emission from Haloes of Simulated Disc Galaxies
- The Stacked Thermal SZ Signal of Locally Brightest Galaxies in Planck Full Mission Data: Evidence for Galaxy Feedback?
- Universal X-ray emissivity of the stellar population in early-type galaxies: unresolved X-ray sources in NGC 3379
- On the OVI Abundance in the Circumgalactic Medium of Low-Redshift Galaxies
- Chandra Survey of Nearby Highly Inclined Disc Galaxies - II: Correlation Analysis of Galactic Coronal Properties
- X-ray Scaling Relation in Early-Type Galaxies: Dark Matter as a Primary Factor in Retaining Hot Gas
- Detection of a luminous hot X-ray corona around the massive spiral galaxy NGC266
- Hot Gaseous Coronae around Spiral Galaxies: Probing the Illustris Simulation
- The Circum-Galactic Medium of MASsive Spirals II: Probing the Nature of Hot Gaseous Halo around the Most Massive Isolated Spiral Galaxies
- Probing the Hot X-ray Corona around the Massive Spiral Galaxy, NGC 6753, Using Deep XMM-Newton observations
- Baryon Budget of the Hot Circumgalactic Medium of Massive Spiral Galaxies
- AGN Driven Weather and Multiphase Gas in the Core of the NGC 5044 Galaxy Group
- Connecting Dark Matter Halos with the Galaxy Center and the Supermassive Black Hole
- Detection of the Missing Baryons toward the Sightline of H1821+643
- EAGLE and Illustris-TNG predictions for resolved eROSITA X-ray observations of the circumgalactic medium around normal galaxies
- Chandra Survey of Nearby Highly Inclined Disc Galaxies - III: Comparison with Hydrodynamical Simulations of Circumgalactic Coronae
- Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
- Probing the Anisotropy of the Milky Way Gaseous Halo-II: sightline toward Mrk509
- The Dearth of Chemically Enriched Warm-Hot Circumgalactic Gas
- The origin of X-ray coronae around simulated disc galaxies
- Thermal Evolution of Supernova Iron in Elliptical Galaxies
- How do atomic code uncertainties affect abundance measurements in the intracluster medium?