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Photometry and kinematics of dwarf galaxies from the Apertif HI survey by Šiljeg, Barbara; Adams, Elizabeth A. K.; Fraternali, Filippo; Hess, Kelley M.; Oosterloo, Tom A.; Marasco, Antonino; Adebahr, Björn; Dénes, Helga; Garrido, Julián; Lucero, Danielle M.; Piña, Pavel E. Mancera; Moss, Vanessa A.; Parra-Royón, Manuel; Ponomareva, Anastasia A.; Sánchez-Expósito, Susana; van der Hulst, J. M. is a scholarly article available to read on EtoBox.

What is Photometry and kinematics of dwarf galaxies from the Apertif HI survey about?

Context. Understanding the dwarf galaxy population in low density environments is crucial for testing the LCDM cosmological model. The increase in diversity towards low mass galaxies is seen as an increase in the scatter of scaling relations such as the stellar mass-size and the baryonic Tully-Fisher relation (BTFR), and is also demonstrated by recent in-depth studies of an extreme subclass of dwarf galaxies of low surface brightness, but large physical sizes, called ultra-diffuse galaxies (UDGs). Aims. We select galaxies from the Apertif HI survey, and apply a constraint on their i-band absolute magnitude to exclude high mass systems. The sample consists of 24 galaxies, and span HI mass ranges of 8.6 < log ($M_{HI}/M_{Sun}$) < 9.7 and stellar mass range of 8.0 < log ($M_*/M_{Sun}$) < 9.7 (with only three galaxies having log ($M_*/M_{Sun}$) > 9). Methods. We determine the geometrical parameters of the HI and stellar discs, build kinematic models from the HI data using 3DBarolo, and extract surface brightness profiles in g-, r- and i-band from the Pan-STARRS 1 photometric survey. Results. We find that, at fixed stellar mass, our HI selected dwarfs have larger optical effective radii

Author

Šiljeg, Barbara; Adams, Elizabeth A. K.; Fraternali, Filippo; Hess, Kelley M.; Oosterloo, Tom A.; Marasco, Antonino; Adebahr, Björn; Dénes, Helga; Garrido, Julián; Lucero, Danielle M.; Piña, Pavel E. Mancera; Moss, Vanessa A.; Parra-Royón, Manuel; Ponomareva, Anastasia A.; Sánchez-Expósito, Susana; van der Hulst, J. M.

Published

2024

Language

EN