Journal
ASTROPHYSICAL JOURNAL
Volume 871, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/aaf424
Keywords
galaxies: bulges; galaxies: elliptical and lenticular, cD; galaxies: kinematics and dynamics; galaxies: photometry; galaxies: spiral; galaxies: structure
Categories
Funding
- Spanish postdoctoral fellowship, Ayudas 1265 para la atraccion del talento investigador. Modalidad 2: jovenes investigadores - Comunidad de Madrid [2016-T2/TIC-2039]
- Spanish Ministry of Economy and Competitiveness - European Regional Development Fund [AYA2016-75808-R]
- Excellence Network MaegNet [AYA2017-90589-REDT]
- SpaceTec-CM: Desarrollo de nuevas tecnologias para instrumentacion espacial en la Comunidad de Madrid [S2013/ICE-2822]
- Alfred P. Sloan Foundation
- U.S. Department of Energy Office of Science
- Center for High-Performance Computing at the University of Utah
- Brazilian Participation Group
- Carnegie Institution for Science
- Carnegie Mellon University
- Chilean Participation Group
- French Participation Group
- Harvard-Smithsonian Center for Astrophysics
- Instituto de Astrofisica de Canarias
- Johns Hopkins University
- Lawrence Berkeley National Laboratory
- Leibniz Institut fur Astrophysik Potsdam
- Max-Planck-Institut fur Astronomie (Heidelberg)
- Max-Planck-Institut fur Astrophysik (Garching)
- Max-Planck-Institut fur Extraterrestrische Physik
- National Astronomical Observatories of China
- New Mexico State University
- New York University
- University of Notre Dame
- Observatario Nacional/MCTI
- Ohio State University
- Pennsylvania State University
- Shanghai Astronomical Observatory
- United Kingdom Participation Group
- Universidad Nacional Autonoma de Mexico
- University of Arizona
- University of Colorado Boulder
- University of Oxford
- University of Portsmouth
- University of Utah
- University of Virginia
- University of Washington
- University of Wisconsin
- Vanderbilt University
- Yale University
- Kavli Institute for the Physics and Mathematics of the Universe/University of Tokyo
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Disky bulges in spiral galaxies are commonly thought to form out of disk materials (mainly) via bar-driven secular processes. They are structurally and dynamically distinct from classical bulges, which are built in violent merger events. We use high-resolution GTC/MEGARA integral-field unit spectroscopic observations of the Sa galaxy NGC 7025, obtained during the MEGARA commissioning run, together with detailed 1D and 2D decompositions of this galaxy's Sloan Digital Sky Survey i-band data to investigate the formation of its disky (bulge) component, which makes up similar to 30% of the total galaxy light. With a Sersic index n similar to 1.80 +/- 0.24, a half-light radius R-e similar to 1.70 +/- 0.43 kpc, and stellar mass M-* similar to (4.34 +/- 1.70) x 10(10) M-circle dot, this bulge dominates the galaxy light distribution in the inner R similar to 15 '' (similar to 4.7 kpc). Measuring the spins (lambda) and ellipticities (epsilon) enclosed within nine different circular apertures with radii R <= R-e, we show that the bulge, which exhibits a spin track of outwardly rising lambda and epsilon, is a fast rotator for all the apertures considered. Our findings suggest that this inner disky component is a pseudo-bulge, consistent with the stellar and dust spiral patterns seen in the galaxy down to the innermost regions but in contrast to the classical bulge interpretation favored in the past. We propose that a secular process involving the tightly wound stellar spiral arms of NGC 7025 may be driving gas and stars out of the disk into the inner regions of the galaxy, building up the massive pseudo-bulge.
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