A reference sample of face-on bulgeless galaxies
arXiv:1902.09892 · doi:10.1093/mnras/stz509
Abstract
We present a list of 220 face-on, almost bulgeless galaxies assumed to be counterparts to the objects from the Reference Flat Galaxy Catalog (RFGC). We selected the Sc, Scd and Sd-type galaxies according to their apparent axial ratio and major standard angular diameter as defined in HyperLEDA. The sample objects are restricted by the radial velocity km/s and a declination of above deg. The morphological composition of our sample is quite similar to that of RFGC. We notice the following common properties of face-on bulgeless galaxies. About half of them have bar-like structures occurring in the whole range of the absolute magnitudes of galaxies: from to mag. An essential part of our sample (27-50%) exhibit distorted spiral patterns. The galaxies do not show significant asymmetry in numbers of the "S"- and "Z"-like spin orientation. The mean (pseudo)bulge-to-total mass ratio for the sample is estimated as 0.11. Due to a negligible internal extinction, low-light background, and small projection effect, the face-on Sc-Sd discs are suitable objects to recognize their central nuclei as moderate-mass BH candidates. About 40-60% of the galaxies have distinct unresolved nuclei, and their presence steeply depend on the luminosity of the host galaxy.
11 pages, 3 tables, 6 figures, accepted for publication in MNRAS
References in corpus (19)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- The Seventh Data Release of the Sloan Digital Sky Survey
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
- Nuclear Activity in Nearby Galaxies
- 2MASS Extended Source Catalog: Overview and Algorithms
- HyperLEDA. III. The catalogue of extragalactic distances
- The Pan-STARRS1 Surveys
- A Catalog of Bulge+Disk Decompositions and Updated Photometry for 1.12 Million Galaxies in the Sloan Digital Sky Survey
- A Low-Mass Central Black Hole in the Bulgeless Seyfert 1 Galaxy NGC 4395
- Bulgeless Giant Galaxies Challenge our Picture of Galaxy Formation by Hierarchical Clustering
- The Next Generation Virgo Cluster Survey. XXIII. Fundamentals of nuclear star clusters over seven decades in galaxy mass
- Astrophysically Motivated Bulge-Disk Decompositions of SDSS Galaxies
- Galaxy And Mass Assembly (GAMA): relations of bulges, discs and spheroids
- Updating the (Supermassive Black Hole Mass) - (Spiral Arm Pitch Angle) Relation: A Strong Correlation for Galaxies with Pseudobulges
- The local Tully-Fisher relation for dwarf galaxies
- The Demographics of galactic bulges in the SDSS database
- Properties of Disks and Bulges of Spiral and Lenticular Galaxies in the Sloan Digital Sky Survey
- Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies
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- H-alpha Images of Ultra-Flat Edge-On Spiral Galaxies