The MeerKAT Fornax Survey VI. The collapse of the galaxy HI Mass Function in Fornax
arXiv:2511.15795 · doi:10.1051/0004-6361/202556734
Abstract
We present the deepest HI mass Function (HIMF) ever measured, outside the Local Group. The observations are part of the MeerKAT Fornax Survey and cover a 4 x 4 deg^2 field, corresponding to ~ Rvir. The 3 detection limit is log(MHI/Msun) = 5.7 for a 50 km/s-wide point source. We detect HI in 35 galaxies and 44 clouds with no optical counterparts. Using deep optical images from the Fornax Deep Survey, we show that the clouds are a distinct population, separated by a four magnitude gap from the faintest HI-detected galaxies. The majority (33 out of 44) of the clouds are associated with the two galaxies with the most HI in the cluster -- NGC 1365 and NGC 1427A, although the clouds contribute a negligible amount to the total MHI budget. By performing a SNR analysis and computing the Rauzy statistic on the HI detections, we demonstrate that our catalogue is complete down log(MHI/Msun) = 6, and we are therefore able to probe the HIMF down to this level. We find an abrupt drop of the number density of HI-detected galaxies at log(MHI/Msun) = 7, signifying a clear absence of galaxies between 6 < log(MHI/Msun) < 7. We use the modified maximum likelihood method to fit a Schechter function down to log(MHI/Msun) > 7, the range where the HIMF follows a power-law. The measured low-mass slope is = -1.31 0.13, with a characteristic knee mass of log(M*/Msun) = 10.52 1.89. The low-mass slope matches the slope in the field, while the knee is defined by a single galaxy and is unconstrained. Below log(MHI/Msun) = 7, there is a sharp departure from a Schechter function, and we report the first robust measurement of the collapse of a HIMF. For the HIMF below log(MHI/Msun) = 7 to follow a power-law, tens of galaxies are needed -- a factor ~ six higher than what is observed. The collapse of the Fornax HIMF is likely due to the rapid removal of HI from low-mass galaxies.
Accepted in Astronomy & Astrophysics. 12 pages, 6 figures
References in corpus (34)
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- Ram Pressure Stripping in High-Density Environments
- SoFiA: a flexible source finder for 3D spectral line data
- The Dawes Review 9: The role of cold gas stripping on the star formation quenching of satellite galaxies
- The cold interstellar medium of galaxies in the Local Universe
- On the origin of the faint-end of the red sequence in high density environments
- The ACS Fornax Cluster Survey. I. Introduction to the Survey and Data Reduction Procedures
- SoFiA 2 -- An automated, parallel HI source finding pipeline for the WALLABY survey
- The Fornax Deep Survey (FDS) with VST. VI. Optical properties of the dwarf galaxies in the Fornax cluster
- The FAST all sky HI survey (FASHI): The first release of catalog
- The Fornax Deep Survey with VST. VIII. Connecting the accretion history with the cluster density
- The Fornax Deep Survey (FDS) with the VST XI. The search for signs of preprocessing between the Fornax main cluster and Fornax A group
- A blind ATCA HI survey of the Fornax galaxy cluster: properties of the HI detections
- Gas sloshing regulates and records the evolution of the Fornax Cluster
- The HI Mass Function and Velocity Width Function of Void Galaxies in the Arecibo Legacy Fast ALFA Survey
- Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
- A MeerKAT view of pre-processing in the Fornax A group
- Eddington's Demon: Inferring Galaxy Mass Functions and other Distributions from Uncertain Data
- Tidal origin of NGC 1427A in the Fornax cluster
- MIGHTEE-HI: The first MeerKAT HI mass function from an untargeted interferometric survey
- The HI mass function of group galaxies in the ALFALFA survey
- The Arecibo Ultra-Deep Survey
- A deep Parkes HI survey of the Sculptor group and filament: HI mass function and environment
- The MeerKAT Fornax Survey II. The rapid removal of HI from dwarf galaxies in the Fornax cluster
- The SRG/eROSITA All-Sky Survey: View of the Virgo Cluster
- The MeerKAT Fornax Survey. III. Ram-pressure stripping of the tidally interacting galaxy NGC 1427A in the Fornax cluster
- The Fornax3D project: The assembly history of massive early-type galaxies in the Fornax cluster from deep imaging and integral field spectroscopy
- The HI mass function in the Parkes HI Zone of Avoidance survey
- NGC 1436: the making of a lenticular galaxy in the Fornax cluster
- The HI Mass Function of the Local Universe: Combining Measurements from HIPASS, ALFALFA and FASHI
- The Ursa Major Association of Galaxies. VI: A relative dearth of gas-rich dwarf galaxies
- The SRG/eROSITA all-sky survey: View of the Fornax galaxy cluster
- The FAST Ursa Major supergroup HI survey (FUMaS): catalog and HI mass function
- The MeerKAT Fornax Survey V. H i kinematics and Fornax cluster membership of the dwarf galaxy ESO 358-60