Study of galaxies in the Lynx-Cancer void. IV. Photometric properties
| Autor: | A. Yu. Kniazev, Yu. A. Perepelitsyna, Simon A. Pustilnik |
|---|---|
| Rok vydání: | 2014 |
| Předmět: |
Physics
Brightness Void (astronomy) Cosmology and Nongalactic Astrophysics (astro-ph.CO) Star formation media_common.quotation_subject HIPASS FOS: Physical sciences Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Astrophysics - Astrophysics of Galaxies Galaxy Photometry (optics) Sky Astrophysics of Galaxies (astro-ph.GA) Astrophysics::Earth and Planetary Astrophysics Surface brightness Instrumentation Astrophysics::Galaxy Astrophysics Astrophysics - Cosmology and Nongalactic Astrophysics media_common |
| Zdroj: | Astrophysical Bulletin. 69:247-265 |
| ISSN: | 1990-3421 1990-3413 |
| DOI: | 10.1134/s1990341314030018 |
| Popis: | We present the results of a photometric study of 85 objects from the updated sample of galaxies residing in the nearby Lynx--Cancer void. We perform our photometry on u, g, r, and i-band images of the Sloan Digital Sky Survey. We determine model-independent galaxy parameters such as the integrated magnitudes and colors, effective radii and the corresponding surface brightness values, optical radii and Holmberg radii. We analyze the radial surface brightness profiles to determine the central brightness values and scale lengths of the model discs. We analyze the colors of the outer parts of the galaxies and compare them with model evolutionary tracks computed using the PEGASE2 software package. This allowed us to estimate the time T_SF elapsed since the onset of star formation, which turned out to be on the order of the cosmological time T_0 for the overwhelming majority of the galaxies studied. However, for 13 galaxies of the sample the time T_SF does not exceed T_0/2 ~ 7 Gyr, and for 7 of them T_SF < 3.5 Gyr. The latter are mostly unevolved objects dominated by low-luminosity galaxies with M_B > -13.2. We use the integrated magnitudes and colors to estimate the stellar masses of the galaxies. We estimate the parameter M(HI)/L_B and the gas mass fractions for void galaxies with known HI-line fluxes. A small subgroup (about 10%) of the gas-richest void galaxies with M(HI)/L_B > 2.5 has gas mass fractions that reach 94-99%. The outer regions of many of these galaxies show atypically blue colors. To test various statistical differences between void galaxies and galaxies from the samples selected using more general criteria, we compare some of the parameters of void galaxies with similar data for the sample of 195 galaxies from the Equatorial Survey (ES) based on a part of the HIPASS blind HI survey. abridged 28 pages, 17 figures, 5 tables. To simplify access to photometrical data, we add in this version all related tables. Published in Astrophysical Bulletin, 2014, vol. 69, p.247-265. Pleiads Press. The MW extinction in estimates of stellar mass was missed. Here we correct this error. This affects stellar mass and gas mass fraction in Table 1 and in Fig.8. The stellar mass median correction is 1.08 |
| Databáze: | OpenAIRE |
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