Article
Astronomy & Astrophysics
Kong You Liow, Steven Rieder, Clare L. Dobbs, Sarah E. Jaffa
Summary: Modelling star formation is challenging, but a grouped star formation method has been introduced and tested in simulations of various physical scales and resolutions, showing its robustness.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
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)
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
David J. Whitworth, Rowan J. Smith, Ralf S. Klessen, Mordecai-Mark Mac Low, Simon C. O. Glover, Robin Tress, Ruediger Pakmor, Juan D. Soler
Summary: Many studies have shown that magnetic fields can suppress star formation in molecular clouds and Milky Way like galaxies. However, most of these studies have focused on fully developed fields at saturation level, and there is little understanding of how weak initial primordial fields affect star formation in low metallicity environments. In this paper, the impact of a weak initial field on low metallicity dwarf galaxies is investigated. High-resolution AREPO simulations are performed, and the results show that the magnetic field has little impact on the global star formation rate (SFR), contrary to some previous studies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Ahmad A. Ali, Clare L. Dobbs, Thomas J. R. Bending, Anne S. M. Buckner, Alex R. Pettitt
Summary: It is still not clear how the galactic environment affects star formation and stellar cluster properties. Previous simulations of Milky Way-mass galaxies have limitations in resolution and accurate feedback. In this study, we conducted zoom-in simulations to re-simulate specific regions of a Milky Way-like galaxy with higher resolution and more accurate modeling. We found that the surface densities of star formation rate and neutral gas follow a certain relation in different regions, with the bar region showing higher values. The bar region also produces the most massive clusters and the inner arm region produces the second most massive clusters. The degree of spatial clustering decreases from the bar to the inter-arm region. These results suggest that young massive clusters, potentially progenitors of globular clusters, may preferentially form near the bar/inner arm compared to the outer arm/inter-arm regions.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Jacob L. Ward, J. M. Diederik Kruijssen, Melanie Chevance, Jaeyeon Kim, Steven N. Longmore
Summary: This paper aims to study the lifecycle of molecular clouds in the Large Magellanic Cloud (LMC) and determines their lifetime to be around 11.8 million years. The study finds that molecular clouds in the LMC are decoupled from galactic dynamics and have short lifetimes regulated by internal processes, while atomic clouds are correlated with galactic dynamical timescales.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
James Wurster, Ian A. Bonnell
Summary: We investigated the role of initial properties on the remnants of molecular cloud collisions. Our study shows that a relatively dense background medium is dynamically important for the evolution of collision remnants. By studying the motions of clouds and remnants through the background, we introduced dynamic boundary conditions and found that the initial velocity has the largest effect on the remnant, affecting its spatial extent and the resulting star clusters. Gas distributions, however, are relatively insensitive to the initial conditions when simulating cloud collisions hydrodynamically in a dynamically important background medium.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
J. Braine, Y. Sun, Y. Shimajiri, F. F. S. van der Tak, M. Fang, Ph. Andre, H. Chen, Y. Gao
Summary: In this study, maps and spectra of the HCN(1-0) and HCO+(1-0) lines in the extreme outer Galaxy were obtained using the Delingha telescope. The aim was to investigate the structure of molecular clouds in subsolar metallicity regions and their relation with star formation. The results showed that the HCN emission is optically thin and the HCO+ emission is stronger, indicating a low-density solution for the dense gas. The correlation between star formation and dense gas was found to be poor.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
K. M. Dutkowska, L. E. Kristensen
Summary: By tracing the molecular outflow emission, the star-forming activity within galactic star-forming regions can be measured. The protostellar outflow emission can be used as a tracer of the star-formation rate (SFR). In this study, a newly developed model is used to relate molecular emission to the SFR, and it is found that the current model underestimates the galactic emission and overestimates the SFR.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
S. Paron, A. Granada, M. B. Areal
Summary: Rare evidence of triggered star formation at large spatial scales involving stellar clusters has been discovered in a Galactic region populated by several open stellar clusters. The discovery suggests that the expansion of the material shell generated by massive stars in Berkeley 7 and UBC 414 clusters could have triggered star formation in some clusters in the past.
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
C. L. Dobbs, T. J. R. Bending, A. R. Pettitt, M. R. Bate
Summary: Our simulations explore the effects of photoionization on cluster formation in different regions of a spiral arm, showing that it has a greater impact in regions with less density and weaker converging flows.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Melanie Chevance, J. M. Diederik Kruijssen, Mark R. Krumholz, Brent Groves, Benjamin W. Keller, Annie Hughes, Simon C. O. Glover, Jonathan D. Henshaw, Cinthya N. Herrera, Jaeyeon Kim, Adam K. Leroy, Jerome Pety, Alessandro Razza, Erik Rosolowsky, Eva Schinnerer, Andreas Schruba, Ashley T. Barnes, Frank Bigiel, Guillermo A. Blanc, Daniel A. Dale, Eric Emsellem, Christopher M. Faesi, Kathryn Grasha, Ralf S. Klessen, Kathryn Kreckel, Daizhong Liu, Steven N. Longmore, Sharon E. Meidt, Miguel Querejeta, Toshiki Saito, Jiayi Sun, Antonio Usero
Summary: The study found that early feedback mechanisms play a crucial role in dispersing GMCs and limiting their star formation efficiency after the onset of star formation, with effects related to the morphological features of galaxies and independent of environmental factors. Additionally, the efficiency at which energy injected by these feedback mechanisms couples with the parent GMC is relatively low.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
F. D. Priestley, P. C. Clark, S. C. O. Glover, S. E. Ragan, O. Feher, L. R. Prole, R. S. Klessen
Summary: The study finds that molecular species commonly assumed to trace the dense, star-forming component of molecular clouds actually exist in material transiently enhanced in density. Only N2H+ exists in detectable quantities above a certain volume density, and N2H+ emission can be used to predict star formation in molecular clouds.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Vineet Rawat, M. R. Samal, D. L. Walker, A. Zavagno, A. Tej, G. Marton, D. K. Ojha, Davide Elia, W. P. Chen, J. Jose, C. Eswaraiah
Summary: Studying the properties of clouds in the early stages of their evolution provides an opportunity to test cluster formation processes. By analyzing the CO, Herschel, and UKIDSS observations of cloud G148.24+00.41, we find that it is a high mass, low dust temperature cloud with a nearly circular shape. Comparing its properties with nearby molecular clouds, we determine that it is similar to the Orion-A molecular cloud in terms of mass, size, and dense gas fraction. Our analysis also suggests that the cloud has the potential to form a cluster in the mass range of 2000-3000 M-circle dot through hierarchical collapse and assembly of gas and stars.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
J. S. Urquhart, C. Figura, J. R. Cross, M. R. A. Wells, T. J. T. Moore, D. J. Eden, S. E. Ragan, A. R. Pettitt, A. Duarte-Cabral, D. Colombo, E. Schuller, T. Csengeri, M. Mattern, H. Beuther, K. M. Menten, F. Wyrowski, L. D. Anderson, P. J. Barnes, M. T. Beltran, S. J. Billington, L. Bronfman, A. Giannetti, J. Kainulainen, J. Kauffmann, M-Y Lee, S. Leurini, S-N X. Medina, F. M. Montenegro-Montes, M. Riener, A. J. Rigby, A. Sanchez-Monge, P. Schilke, E. Schisano, A. Traficante, M. Wieneri
Summary: By studying the role of spiral arms in the star formation process, it was found that the molecular material associated with ATLASGAL clumps is mostly concentrated in the arms, but there was no evidence of enhanced physical parameters near the arms. The results suggest that star formation activities depend more on local environment effects, rather than the influence of spiral arms.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
A. Duarte-Cabral, D. Colombo, J. S. Urquhart, A. Ginsburg, D. Russeil, F. Schuller, L. D. Anderson, P. J. Barnes, M. T. Beltran, H. Beuther, S. Bontemps, L. Bronfman, T. Csengeri, C. L. Dobbs, D. Eden, A. Giannetti, J. Kauffmann, M. Mattern, S-N X. Medina, K. M. Menten, M-Y Lee, A. R. Pettitt, M. Riener, A. J. Rigby, A. Traficante, V. S. Veena, M. Wienen, F. Wyrowski, C. Agurto, F. Azagra, R. Cesaroni, R. Finger, E. Gonzalez, T. Henning, A. K. Hernandez, J. Kainulainen, S. Leurini, S. Lopez, F. Mac-Auliffe, P. Mazumdar, S. Molinari, F. Motte, E. Muller, Q. Nguyen-Luong, R. Parra, J-P Perez-Beaupuits, F. M. Montenegro-Montes, T. J. T. Moore, S. E. Ragan, A. Sanchez-Monge, A. Sanna, P. Schilke, E. Schisano, N. Schneider, S. Suri, L. Testi, K. Torstensson, P. Venegas, K. Wang, A. Zavagno
Summary: By utilizing the (CO)-C-13(2-1) emission from the SEDIGISM survey, a total of 10,663 molecular clouds were studied, with 10,300 having distances and physical properties computed. The study compared scaling relations of clouds from SEDIGISM with other surveys, revealing trends in mass, size, surface density, and velocity dispersion for clouds with ongoing high-mass star formation. The Galactic distribution of extreme clouds was found to be only marginally different from the overall cloud population, with the largest, turbulent, and high-mass star-forming clouds deviating significantly.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
F. Schuller, J. S. Urquhart, T. Csengeri, D. Colombo, A. Duarte-Cabral, M. Mattern, A. Ginsburg, A. R. Pettitt, F. Wyrowski, L. Anderson, F. Azagra, P. Barnes, M. Beltran, H. Beuther, S. Billington, L. Bronfman, R. Cesaroni, C. Dobbs, D. Eden, M-Y Lee, S-N X. Medina, K. M. Menten, T. Moore, F. M. Montenegro-Montes, S. Ragan, A. Rigby, M. Riener, D. Russeil, E. Schisano, A. Sanchez-Monge, A. Traficante, A. Zavagno, C. Agurto, S. Bontemps, R. Finger, A. Giannetti, E. Gonzalez, A. K. Hernandez, T. Henning, J. Kainulainen, J. Kauffmann, S. Leurini, S. Lopez, F. Mac-Auliffe, P. Mazumdar, S. Molinari, F. Motte, E. Muller, Q. Nguyen-Luong, R. Parra, J-P Perez-Beaupuits, P. Schilke, N. Schneider, S. Suri, L. Testi, K. Torstensson, V. S. Veena, P. Venegas, K. Wang, M. Wienen
Summary: The SEDIGISM survey utilizes the APEX telescope to map the structure, excitation, and dynamics of the interstellar medium, providing insights into the large-scale distribution of cold molecular gas in the Milky Way. Results show that approximately 60% of the molecular gas is associated with the spiral arms, with 13CO emission concentrated in a small number of specific complexes rather than evenly distributed along the arms.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Daniel L. Walker, Steven N. Longmore, John Bally, Adam Ginsburg, J. M. Diederik Kruijssen, Qizhou Zhang, Jonathan D. Henshaw, Xing Lu, Joao Alves, Ashley T. Barnes, Cara Battersby, Henrik Beuther, Yanett A. Contreras, Laura Gomez, Luis C. Ho, James M. Jackson, Jens Kauffmann, Elisabeth A. C. Mills, Thushara Pillai
Summary: The translation details the active star formation phenomenon within the massive and dense molecular cloud G0.253+0.016 in the Milky Way, revealing numerous protostars with potential to develop into intermediate and high-mass stars.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
P. Salas, M. R. Rugel, K. L. Emig, J. Kauffmann, K. M. Menten, F. Wyrowski, A. G. G. M. Tielens
Summary: The electron density (ne) and gas temperature in the envelope of the integral shaped filament (ISF) in the Orion A molecular cloud were directly measured using carbon radio recombination lines and far-infrared lines of C. The results showed a gas density of around 5×10^3 cm^-3, electron density ranging from 0.65 to 0.95 cm^-3, and an ionization fraction of less than 3×10^-3.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Dan P. Clemens, Thushara G. S. Pillai, Anneliese M. Rilinger, Catherine C. Espaillat
Summary: Wide-field near-infrared polarimetry was used to study the disk systems around two brown dwarfs and two young stellar objects in Taurus. Significant intrinsic polarization was detected from one brown dwarf and both young stellar objects, and their disk orientations were found to be consistent with published imaging results.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
G. Parmentier, A. Pasquali
Summary: The article presents a novel approach to understanding the phenomenon of star cluster multiple populations. By studying the formation and dispersal of failed cores in cluster-forming clumps, the authors propose that these failed cores play a crucial role in regulating the gas density and star formation rates of clusters. They identify three main parameters that shape the star formation history of a clump and use their model to analyze the Orion Nebula Cluster progenitor clump. The authors caution that the star formation histories of starburst clusters may contain hidden peaks masked by uncertainties in stellar age. They also draw parallels between their findings and the diverse morphologies observed in old globular clusters.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
J. S. Urquhart, M. R. A. Wells, T. Pillai, S. Leurini, A. Giannetti, T. J. T. Moore, M. A. Thompson, C. Figura, D. Colombo, A. Y. Yang, C. Koenig, F. Wyrowski, K. M. Menten, A. J. Rigby, D. J. Eden, S. E. Ragan
Summary: ATLASGAL is a dust survey that identifies dense molecular clumps in the inner Galactic plane. The physical properties and evolutionary sequence of these clumps are studied using follow-up observations and complementary surveys. The analysis of the data shows that the star formation process is continuous and the different observational stages do not represent fundamentally different stages or changes in the physical mechanisms involved. Comparing the results with other star formation tracers confirms the reliability of the classification and reveals the early indication of star formation through molecular outflows.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Sudeshna Patra, Neal J. Evans, Kee-Tae Kim, Mark Heyer, Jens Kauffmann, Jessy Jose, Manash R. Samal, Swagat R. Das
Summary: In this study, we mapped HCN and HCO+ (J = 1 -> 0) line emission towards star-forming regions in the outer Milky Way. We found that HCN and HCO+ correlate better with millimeter-wave emission than with the extinction criterion. Furthermore, we observed that HCN and HCO+ trace dense gas in high column density regions better than (CO)-C-13. The concentration of HCO+ is less in outer Galaxy targets compared to inner Galaxy samples, suggesting a possible influence of metallicity on dense gas tracers.
ASTRONOMICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Laura A. Busch, Denise Riquelme, Rolf Guesten, Karl M. Menten, Thushara G. S. Pillai, Jens Kauffmann
Summary: This study investigates the interaction between cloud complexes in the central molecular zone (CMZ) of our Galaxy. The results suggest that there is evidence of cloud-cloud interactions in G1.3, while the low-velocity and high-velocity components in G1.6 are coincidental observations. The kinetic temperatures and H2 volume densities are similar in both complexes, and the chemical composition is consistent with other sources.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Daniel Callanan, Steven N. Longmore, Cara Battersby, H. Perry Hatchfield, Daniel L. Walker, Jonathan Henshaw, Eric Keto, Ashley Barnes, Adam Ginsburg, Jens Kauffmann, J. M. Diederik Kruijssen, Xing Lu, Elisabeth A. C. Mills, Thushara Pillai, Qizhou Zhang, John Bally, Natalie Butterfield, Yanett A. Contreras, Luis C. Ho, Katharina Immer, Katharine G. Johnston, Juergen Ott, Nimesh Patel, Volker Tolls
Summary: We present an overview and data release of the spectral line component of the SMA Large Program, CMZoom. The study observed various transitions of molecules in the Central Molecular Zone (CMZ), analyzing source kinematics and the presence of proto-stellar outflows. No high-velocity compact clouds (HVCCs), which could indicate the presence of intermediate mass black holes, were found in the survey area.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Kazunori Akiyama, Jens Kauffmann, Lynn D. Matthews, Kotaro Moriyama, Shoko Koyama, Kazuhiro Hada
Summary: The proposed ngEHT concept aims to image astronomical sources in unprecedented detail and improve the image dynamic ranges by extending the EHT. The ngEHT will utilize large aperture telescopes to connect less sensitive stations and form a dense network across the planet. LST and AtLAST, two planned large radio telescopes in Chile, with a diameter of 50 meters, will play a key role in enabling transformative science cases with next-generation millimeter/submillimeter VLBI arrays.
Article
Astronomy & Astrophysics
Jens Kauffmann, Ganesh Rajagopalan, Kazunori Akiyama, Vincent Fish, Colin Lonsdale, Lynn D. Matthews, Thushara G. S. Pillai
Summary: The Haystack Telescope is a 37 m diameter antenna capable of millimeter-wave observations. It serves as a radar sensor for space situational awareness and is used for research by MIT Haystack Observatory. Ongoing testing is preparing for its inclusion in the Event Horizon Telescope array and its use as a single-dish research telescope. Its addition would substantially improve the image quality of the EHT array.
Proceedings Paper
Engineering, Aerospace
Peter L. Kurczynski, Michael D. Johnson, Sheperd S. Doeleman, Kari Haworth, Eliad Peretz, Tirupati Kumara Sridharan, Byran Bilyeu, Lindy Blackburn, Don Boroson, Alexandra Brosius, Richard Butler, Dave Caplan, Koushik Chatterjee, Peter Cheimets, Daniel D'Orazio, Thomas M. Essinger-Hileman, Peter Galison, Ronald Gamble, Shahar Hadar, Tiffany Hoerbelt, Hua Jiao, Jens Kauffmann, Robert Lafon, Chung-Pei Ma, Gary Melnick, Nathan R. Newbury, Scott Noble, Daniel Palumbo, Lenny Paritsky, Dominic Pesce, Leonid Petrov, Jeff Piepmeier, Christopher J. Roberts, Bryon Robinson, Curt Shieler, Jeffrey Small, Neal Spellmeyer, Paul Tiede, Jaye Verniero, Jade Wang, Maciek Wielgus, Ed Wollack, George N. Wong, Guangning Yang
Summary: This article presents the highlights and overview of the Event Horizon Explorer (EHE) mission concept, discussing its feasibility and outlining scientific goals, key technologies, and engineering challenges. Furthermore, an assessment of their technological readiness and overall suitability for a NASA Medium Explorer (MIDEX) class mission is provided.
SPACE TELESCOPES AND INSTRUMENTATION 2022: OPTICAL, INFRARED, AND MILLIMETER WAVE
(2022)