Unveiling an old disk around a massive young leaking blueberry in SDSS-IV MaNGA
arXiv:2203.04207 · doi:10.3847/1538-4357/ac5c4b
Abstract
Extreme emission-line galaxies, such as blue compact dwarfs (BCDs), Green Peas (GPs) and blueberries in the local Universe are the potential candidates to understand the nature of galaxies that re-ionized the early Universe. Being low-mass, metal-poor starburst systems they are understood as local analogs of the high redshift Lyman Continuum (LyC) and Lyman- emitters (LAEs). Even with their proximity to us, we know little about their spatially resolved properties, most of the blueberries and GPs are indeed compact, remain unresolved. Here, we report the detection of a disk-like lower-surface brightness (LSB) stellar host with very old population around a blueberry LAE system using broad i-band imaging and integral field spectroscopic data from SDSS and SDSS-IV MaNGA surveys, respectively. The LSB stellar host is structurally similar to that observed around15 local starburst BCDs. Furthermore, the kinematics of the studied blueberry source bear sign of misalignment between the gas and stellar components. Our findings establish an intriguing thread connecting the blueberry and an LSB disk with old stellar population, and suggest that blueberries and their high redshift counterparts such as GPs do not represent peculiar cases of dwarf galaxy evolution. In fact, with respect to the structural properties of their host galaxies, they are compatible with a common evolutionary track of the main population of local BCDs.
Accepted for publication in ApJ
References in corpus (28)
- The 2.5 m Telescope of the Sloan Digital Sky Survey
- Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
- Galaxy Zoo 1 : Data Release of Morphological Classifications for nearly 900,000 galaxies
- The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey
- The SDSS-IV MaNGA Sample: Design, Optimization, and Usage Considerations
- Effects of Supernova Feedback on the Formation of Galaxy Disks
- Lyman-alpha spectral properties of five newly discovered Lyman continuum emitters
- Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence
- Feedback-regulated star formation and escape of LyC photons from mini-haloes during reionisation
- Q1549-C25: A Clean Source of Lyman-Continuum Emission at
- Why stellar feedback promotes disc formation in simulated galaxies
- Blueberry galaxies: the lowest mass young starbursts
- On the Origin of Exponential Galaxy Disks
- Extremely metal-poor star-forming galaxies. New detections and general morphological and photometric properties
- New HI scaling relations to probe the HI content of galaxies via global HI-deficiency maps
- SDSS-IV MaNGA: Properties of galaxies with kinematically decoupled stellar and gaseous components
- Linking Ly-alpha and Low-Ionization Transitions at Low Optical Depth
- How galaxies lose their angular momentum
- Low-redshift compact star-forming galaxies as analogues of high-redshift star-forming galaxies
- A deep wide survey of faint low surface brightness galaxies in the direction of the Coma cluster of galaxies
- AstroSat detection of Lyman continuum emission from a z=1.42 galaxy
- Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. II. Extending the mass-metallicity relation to the range z=0.89-1.24
- The Origin of Extended Disk Galaxies at z=2
- Modelling a bright z = 6 galaxy at the faint end of the AGN luminosity function
- A Population of Metal-Poor Galaxies with ~L* Luminosities at Intermediate Redshifts
- The Atomic Gas Mass of Green Pea Galaxies
- Tidal interaction, star formation and chemical evolution in blue compact dwarf galaxy Mrk 22
- SDSS-IV MaNGA: an observational evidence of density bounded region in a Lyman- emitter