2014/12/05 by Gerold Busch, G. Busch, Semir Smajić +13 · 1 citation
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Astrophysics #Bulge #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #Luminosity #Physics #QSOS #Redshift #Spiral galaxy #Star formation #Stellar population #Supermassive black hole #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201425261
published as A&A 575, A128 (2015) · 16 pages, 11 figures, submitted to A&A, comments welcome
arxiv created 2014/12/05 · openalex publication_date 2015/03/01 · arxiv updated 2015/03/11 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Circumnuclear star formation and active galactic nucleus (AGN) feedback is believed to play a critical role in galaxy evolution. The low-luminosity quasi-stellar object (LLQSO) sample that contains 99 of the closest AGN with redshift z ≤ 0.06 fills the gap between the local AGN population and high-redshift QSOs that is essential to understand the AGN evolution with redshift. In this paper, we present the results of the near-infrared H- and K- integral field spectroscopy of the inner kiloparsecs of the LLQSO HE 1029-1831 with SINFONI. Line maps show that ionized hydrogen gas is located in spiral arms within the stellar bar and in a circumnuclear ring. Line fluxes and diagnostic line ratios indicate recent or ongoing star formation in the circumnuclear region and the presence of young and intermediate-age stellar populations in the bulge. In particular, we find traces of an intense starburst in the circumnuclear region that has begun around 100 Myr ago but has declined to a fraction of the maximum intensity now. We estimate the dynamical bulge mass and find that the galaxy follows published MBH − Mbulge relations. However, bulge-disk decomposition of the K-band image with Budda reveals that HE 1029-1831 does not follow the MBH − Lbulge relations of inactive galaxies. We conclude that the deviation from MBH − Lbulge relations of inactive galaxies in this source is instead caused by young stellar populations and not by an undermassive black hole.