Article
Astronomy & Astrophysics
Jorge Moreno, Paul Torrey, Sara L. Ellison, David R. Patton, Connor Bottrell, Asa F. L. Bluck, Maan H. Hani, Christopher C. Hayward, James S. Bullock, Philip F. Hopkins, Lars Hernquist
Summary: The study shows that close encounters in interacting galaxies significantly increase cool gas budgets, leading to enhanced star formation. Additionally, galaxies with high global star formation rates experience intense nuclear star formation enhancement in the central region, while those with low global SFR are suppressed in the central region.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
M. Romano, A. Nanni, D. Donevski, M. Ginolfi, G. C. Jones, I. Shivaei, Junais, D. Salak, P. Sawant
Summary: The physical properties of star-formation-driven outflows in a sample of 29 local dwarf galaxies were characterized in this study. Atomic outflow signatures were detected in the high-velocity tails of 11 sources, while weaker outflows were detected in the average stacked spectrum. The outflow rates were found to be comparable to the star-formation rates of the galaxies, with a significant amount of gas escaping into the intergalactic medium (IGM).
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
A. Audibert, F. Combes, S. Garcia-Burillo, L. Hunt, A. Eckart, S. Aalto, V Casasola, F. Boone, M. Krips, S. Viti, S. Muller, K. Dasyra, P. van der Werf, S. Martin
Summary: ALMA observations of NGC1808 reveal a nuclear spiral and a circumnuclear disk, with detections of dense gas line tracers like HCN, HCO+, and CS. Presence of an active galactic nucleus is indicated at the nucleus, with regular rotation observed within a radius of 400 pc, except for non-circular motions in the nuclear spiral arms. Potential weak outflow attributed to AGN feedback is observed along with a molecular outflow likely due to supernovae feedback at >= 250 pc in the NE direction, connected to a kpc-scale superwind.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Bronwyn Reichardt Chu, Deanne B. Fisher, Nikole M. Nielsen, John Chisholm, Marianne Girard, Glenn G. Kacprzak, Alberto Bolatto, Rodrigo Herrera-Camus, Karin Sandstrom, Miao Li, Ryan Rickards Vaught, Daniel K. McPherson
Summary: Star formation-driven outflows in the starbursting disc galaxy IRAS08339+6517 at z similar to 0.02 were studied using the Keck Cosmic Web Imager. A new method was developed to determine the characteristics of the outflows, and it was found that the outflows exist in a large portion of the galaxy, consistent with the trends expected from energy-driven feedback models.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Y. I. Izotov, T. X. Thuan, N. G. Guseva
Summary: The compact star-forming galaxies reported in this study exhibit characteristics of young starburst ages and high ionization radiation, with most being low-metallicity objects. Their spectra show features such as Wolf-Rayet lines, indicating that stellar ionization radiation alone is not sufficient to produce such strong emission. Models suggest non-uniform density distributions in these galaxies, with different lines emitted in channels of varying density.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Y. I. Izotov, T. X. Thuan, N. G. Guseva
Summary: Through optical spectroscopy of the metal-poor dwarf star-forming galaxy J2229+2725, obtained using the LBT/MODS, it was found that this galaxy deviates significantly from the luminosity-metallicity relation defined by most SFGs in the SDSS. With extremely low oxygen abundance, very young starburst, and highly active ongoing star formation, J2229+2725 exhibits properties that are most extreme among the lowest metallicity SFGs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
N. G. Guseva, T. X. Thuan, Y. I. Izotov
Summary: The spectral time variations of candidate luminous blue variable (cLBV) stars in low-metallicity star-forming galaxies DDO 68 and PHL 293B were examined. It was found that LBV in DDO 68 experienced an outburst, while the cLBV in PHL 293B remained relatively constant over a 16-year period.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
F. Valentino, E. Daddi, A. Puglisi, G. E. Magdis, V Kokorev, D. Liu, S. C. Madden, C. Gomez-Guijarro, M-Y Lee, I Cortzen, C. Circosta, I Delvecchio, J. R. Mullaney, Y. Gao, R. Gobat, M. Aravena, S. Jin, S. Fujimoto, J. D. Silverman, H. Dannerbauer
Summary: The study found detectable nuclear activity in about 30% of the sample, with the presence of dusty tori influencing the IR spectral energy distribution of galaxies, but with minimal effects on the excitation of molecular gas.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Alvaro Segovia Otero, Florent Renaud, Oscar Agertz
Summary: This study explores the effects of galaxy mergers and morphological transformations on star formation modes, finding that major mergers trigger multiple starburst episodes and enhance the overall star formation rate.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
K. Kouroumpatzakis, A. Zezas, A. Maragkoudakis, S. P. Willner, P. Bonfini, M. L. N. Ashby, P. H. Sell, T. H. Jarrett
Summary: This study presents new H alpha photometry for the Star Formation Reference Survey (SFRS) and calibrations of H alpha-based star-formation rates, considering the impact of different correction factors. The research compares SFR estimates derived from different methods, studies the dependence of the radio-to-H alpha emission ratio, and quantifies the correlation between galaxy metallicity and extinction.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Jaeyeon Kim, Melanie Chevance, J. M. Diederik Kruijssen, Andreas Schruba, Karin Sandstrom, Ashley T. Barnes, Frank Bigiel, Guillermo A. Blanc, Yixian Cao, Daniel A. Dale, Christopher M. Faesi, Simon C. O. Glover, Kathryn Grasha, Brent Groves, Cinthya Herrera, Ralf S. Klessen, Kathryn Kreckel, Janice C. Lee, Adam K. Leroy, Jerome Pety, Miguel Querejeta, Eva Schinnerer, Jiayi Sun, Antonio Usero, Jacob L. Ward, Thomas G. Williams
Summary: Feedback from massive stars is crucial in molecular cloud evolution. The embedded phase of massive star formation lasts 2-7 million years, with the region heavily obscured in the first half and partially exposed in the second half. After the cloud disperses, ongoing star formation is no longer traced by 24 emission, but can be detected through ambient CO-dark gas emissions for 2-9 million years. Future JWST observations will enable routine measurements across nearby galaxies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
W. E. Banda-Barragan, M. Brueggen, V Heesen, E. Scannapieco, J. Cottle, C. Federrath, A. Y. Wagner
Summary: Galactic winds play a crucial role in transporting material out of galaxies, and simulations show that radiative heating and cooling create a complex multiphase flow with rain-like morphology. The interplay between shock heating, turbulence, and radiative processes leads to the formation of dense gas cloudlets and filaments, explaining the presence of high-velocity HI gas in the Galactic Center outflow. This cycle sustains fast-moving dense gas by aiding condensation from warm clouds and the hot wind, with most of the mass concentrated in the dense gas phases.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Kearn Grisdale
Summary: The choice of star formation criteria impacts both galactic and giant molecular cloud scales in a Milky Way-like galaxy simulation. Using a turbulent, self-gravitating star formation criteria leads to increased gas density and larger cloud sizes, affecting the location and distribution of star formation. Despite the differences, relationships between cloud properties remain unaffected.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Anqi Li, Filippo Fraternali, Antonino Marasco, Scott C. Trager, Gabriele Pezzulli, Pavel E. Mancera Pina, Marc A. W. Verheijen
Summary: We used a dynamical model of galactic fountain to study the extraplanar gas in NGC 2403. The model suggests a total EPG mass of 4.7 x 10(8) M-? with a typical scale height of 1 kpc and a vertical gradient of the rotation velocity of -10.0 km s(-1) kpc(-1). The accretion rate from the condensation of the inner hot CGM inferred by the model is approximately equal to the star-formation rate in this galaxy.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Glen H. Hunter, Paul C. Clark, Simon C. O. Glover, Ralf S. Klessen
Summary: In this study, the impact of collision speed, magnetic field inclination, and resolution on the star formation rate (SFR) in cloud-cloud collisions is investigated. A factor of 2-3 increase in the SFR is found compared to no collision simulations, with high collisional velocities, parallel magnetic field and collision axis orientation, and lower resolution leading to earlier star formation. The alignment of velocity and magnetic field is consistent in low-density environments but becomes more perpendicular as density increases, indicating the compression of the magnetic field by collapsing gas.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)