Detalles de publicación
PP 026113
Serendipitous discovery of an almost-dark galaxy in the Virgo Cluster
(1) Instituto de Astrofísica de Canarias, Vía Láctea S/N, E-38205 La Laguna, Spain
(2) Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Spain
(3) Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700AV Groningen, The Netherlands
(4) Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
(5) Department of Astronomy and the DiRAC Institute, University of Washington, 3910 15th Avenue, NE, Seattle, WA 98195, USA
(6) Bernoulli Institute of Mathematics, Computer Science and Artificial Intelligence, University of Groningen, Groningen, The Netherlands
(7) Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain
(8) Light Bridges, Observatorio del Teide, Carretera del Observatorio s/n, E-38500 Guimar, Tenerife, Canarias, Spain
Abstract:Analogues of extreme Local Group galaxies with very low surface brightness and large effective radii must exist elsewhere, still hidden due to current detection limits. We report the serendipitous discovery of a low-mass almost-dark galaxy TTT J1237327+143535 in the Virgo Cluster, observed using the Two-meter Twin Telescope at the Teide Observatory. TTT J1237327+143535 has a central surface brightness of $27.9 \pm 0.2 \, \mathrm{mag arcsec}^{-2}$ in the $g'$-band, an effective radius of $0.9 \pm 0.1 \, \mathrm{kpc}$, and a total stellar mass of $(2.2 \pm 0.4) \times 10^6 \, \mathrm{M_\odot}$. Its effective radius and absolute magnitude are similar to those of galaxies And XXI and And XXIII. The discovery of this extremely low surface brightness, extended, low-mass galaxy suggests the existence of a significant population of almost-dark galaxies in the Virgo Cluster. An in-depth analysis of the Next Generation Virgo Cluster survey, as well as upcoming Rubin Data Releases and the 10-year Rubin Legacy Survey of Space and Time are expected to reveal large samples of this extreme galaxy population, which offers insights on galaxy formation in extreme conditions.