Article
Astronomy & Astrophysics
F. Fontani, L. Colzi, L. Bizzocchi, V. M. Rivilla, D. Elia, M. T. Beltran, P. Caselli, L. Magrini, A. Sanchez-Monge, L. Testi, D. Romano
Summary: This paper presents a new observational project called CHEMOUT, which aims to investigate the chemical composition in star-forming regions of the outer Galaxy. The results show that organic molecules and tracers of protostellar activity are ubiquitous in the low metallicity environment of the outer Galaxy.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
H. Nguyen, M. R. Rugel, C. Murugeshan, K. M. Menten, A. Brunthaler, J. S. Urquhart, R. Dokara, S. A. Dzib, Y. Gong, S. Khan, S-N X. Medina, G. N. Ortiz-Leon, W. Reich, F. Wyrowski, A. Y. Yang, H. Beuther, W. D. Cotton, J. D. Pandian
Summary: Class II methanol masers are clear indicators of recent high-mass star formation and the Global View on Star Formation (GLOSTAR) survey provides a complete catalogue outlining the distribution of star formation in the Galaxy, the number of young star-forming cores, and their physical conditions. This survey mapping the Galactic mid-plane in the radio continuum, 6.7 GHz methanol line, 4.8 GHz formaldehyde line, and radio recombination lines detected a total of 554 methanol masers, cataloguing their positions, velocity components, and integrated fluxes. It is the most sensitive survey for methanol masers to date.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
F. Meng, A. Sanchez-Monge, P. Schilke, A. Ginsburg, C. DePree, N. Budaiev, D. Jeff, A. Schmiedeke, A. Schwoerer, V. S. Veena, Th Moeller
Summary: This study aims to characterize the properties of HII regions in the molecular cloud Sagittarius B2, with a focus on identifying and analyzing various UCHIT regions in the complex to reveal different evolutionary stages of the cloud.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
M. Wienen, C. M. Brunt, C. L. Dobbs, D. Colombo
Summary: Expanding (sub)millimetre capabilities to high angular resolution with interferometers enables the resolution of giant molecular clouds in nearby galaxies. By remapping CO-C-12 data along the Perseus spiral arm in the Milky Way, at a common distance to an observer outside the galaxy, important insights into the structure of the arm, including thickness, centroid position, and mass distribution, were determined.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
A. Traficante, B. M. Jones, A. Avison, G. A. Fuller, M. Benedettini, D. Elia, S. Molinari, N. Peretto, S. Pezzuto, T. Pillai, K. L. J. Rygl, E. Schisano, R. J. Smith
Summary: The mechanism of the formation of the most massive stars is still not completely understood. The SQUALO project, an ALMA survey, was introduced to investigate the properties of 13 massive clumps in different evolutionary stages. The results obtained from the survey show evidence of fragmentation and correlation between the physical properties of the fragments and their parent clumps.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Gisela N. Ortiz-Leon, Karl M. Menten, Andreas Brunthaler, Timea Csengeri, James S. Urquhart, Friedrich Wyrowski, Yan Gong, Michael R. Rugel, Sergio A. Dzib, Aiyuan Yang, Hans Nguyen, William D. Cotton, Sac Nicte X. Medina, Rohit Dokara, Carsten Koenig, Henrik Beuther, Jagadheep D. Pandian, Wolfgang Reich, Nirupam Roy
Summary: The GLOSTAR survey observed methanol tracers of high-mass young stellar objects in the Cygnus X complex, detecting thirteen sources with Class II methanol maser emission and one with methanol absorption. Most of these masers are concentrated in the DR21 ridge and W75N regions, associated with (sub)millimeter dust continuum emission.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
O. L. Ryabukhina, M. S. Kirsanova, C. Henkel, D. S. Wiebe
Summary: In this study, observations and astrochemical modeling were used to investigate the physical properties, collapse features, and chemical ages of dense clumps in an interstellar filament. The results suggest rapid interstellar matter accumulation and collapse over a time scale of approximately 10(5) years, which is important for understanding the evolution of interstellar matter.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
F. Fontani, A. Schmiedeke, A. Sanchez-Monge, L. Colzi, D. Elia, V. M. Rivilla, M. T. Beltran, L. Bizzocchi, P. Caselli, L. Magrini, D. Romano
Summary: The study reveals that the chemical properties of the outer star-forming regions of the Galaxy are similar to those of the inner and local regions. Methanol (CH3OH) is detected in the observed targets, and its emission is associated with an extended envelope, indicating that it mainly comes from a cold and quiescent region. The relative abundance of CH3OH shows good correlations with that of H2CO, but not with HCO. These findings have significant implications for understanding the organic and possibly pre-biotic chemistry in the outermost star-forming regions of the Galaxy.
ASTRONOMY & ASTROPHYSICS
(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
F. Fontani, L. Colzi, E. Redaelli, O. Sipilae, P. Caselli
Summary: Studying the chemical processes in high-mass star-forming regions is crucial for understanding the chemical heritage of the Solar System and most stellar systems in the Galaxy. The abundance ratios of HCNH+ can be useful astrochemical tools to distinguish between different evolutionary phases in the process of star formation.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
X. D. Tang, C. Henkel, K. M. Menten, Y. Gong, C-H R. Chen, D. L. Li, M-Y Lee, J. G. Mangum, Y. P. Ao, S. Muehle, S. Aalto, S. Garcia-Burillo, S. Martin, S. Viti, S. Muller, F. Costagliola, H. Asiri, S. A. Levshakov, M. Spaans, J. Ott, C. M. Impellizzeri, Y. Fukui, Y. X. He, J. Esimbek, J. J. Zhou, X. W. Zheng, X. Zhao, J. S. Li
Summary: The study on the kinetic temperature structure of two massive star-forming regions in the Large Magellanic Cloud found that the dense gas's kinetic temperature is influenced by embedded infrared sources and/or young stellar objects. Lower temperatures were measured at the outskirts of H2CO-traced dense gas distributions, while turbulence may be correlated with higher kinetic temperatures.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Vipin Kumar, S. Vig, V. S. Veena, S. Mohan, S. K. Ghosh, A. Tej, D. K. Ojha
Summary: The star-forming activity in the H ii region RCW 42 has been studied using observations at multiple wavebands. A large expanse of the H ii region, spanning 20 x 15 pc(2), has been identified, along with the estimation of average electron density and ionization fraction. An extended green object and several young stellar objects have also been detected in the region.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
M. Juvela, E. Mannfors, T. Liu, L. Toth
Summary: This study evaluated the physical conditions within massive star-forming clouds using magnetohydrodynamic simulation data and synthetic observations, with a focus on the potential of the ngVLA interferometer. The ngVLA proved capable of providing accurate data on small-scale structures and physical states in high-mass star-forming regions at kiloparsec distances.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
M. Durjasz, M. Szymczak, P. Wolak, A. Bartkiewicz
Summary: This study aimed to search for 12.2 GHz methanol emission in 6.7 GHz methanol masers and revealed its detection in 36 high-mass young stellar objects. The flux density ratio between 6.7 and 12.2 GHz exhibited significant variability among sources, with a median value of 5.1. Comparison with historical data suggested noticeable (>50%) variability in methanol maser emission over the past decade.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Clara M. Pennock, Jacco Th van Loon, Miroslav D. Filipovic, Heinz Andernach, Frank Haberl, Roland Kothes, Emil Lenc, Lawrence Rudnick, Sarah White, Claudia Agliozzo, Sonia Anton, Ivan Bojicic, Dominik J. Bomans, Jordan D. Collier, Evan J. Crawford, Andrew M. Hopkins, Kanapathippillai Jeganathan, Patrick J. Kavanagh, Barbel S. Koribalski, Denis Leahy, Pierre Maggi, Chandreyee Maitra, Josh Marvil, Michal J. Michalowski, Ray P. Norris, Joana M. Oliveira, Jeffrey L. Payne, Hidetoshi Sano, Manami Sasaki, Lister Staveley-Smith, Eleni Vardoulaki
Summary: The analysis of a new radio continuum image of the Large Magellanic Cloud presents a catalog of sources and discusses various detections of celestial objects and their characteristics.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Kenji Furuya, Takashi Tsukagoshi, Chunhua Qi, Hideko Nomura, L. Ilsedore Cleeves, Seokho Lee, Tomohiro C. Yoshida
Summary: By observing the TW Hya disk, the first detection of oxygen isotope fractionation in HCO+ gas in a protoplanetary disk is reported. The study suggests that optically thin lines of HCO+ isotopologues are useful tracers of CO isotopic ratios.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Takashi Tsukagoshi, Hideko Nomura, Takayuki Muto, Ryohei Kawabe, Kazuhiro D. Kanagawa, Satoshi Okuzumi, Shigeru Ida, Catherine Walsh, Tom J. Millar, Sanemichi Z. Takahashi, Jun Hashimoto, Taichi Uyama, Motohide Tamura
Summary: In this study, a high-resolution multiband analysis of the protoplanetary disk around TW Hya using ALMA long baseline data is presented. Two methods are employed to reconstruct the images and investigate the spectral index distribution. The results show that the multifrequency synthesis imaging method can accurately reproduce the frequency dependence of the continuum emission, while the image-oriented method provides consistent results but with lower resolution.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Tomomi Shimoikura, Kazuhito Dobashi, Naomi Hirano, Fumitaka Nakamura, Tomoya Hirota, Tomoaki Matsumoto, Kotomi Taniguchi, Yoshito Shimajiri
Summary: Observations of the GGD 12-15 region reveal a massive clump with characteristics similar to star cluster formation. A bipolar molecular outflow, driven by a constituent star of the cluster, indicates gravitational contraction and rotation of the clump. The velocity structure strongly suggests an infalling motion in the region.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Takahiro Ueda, Akimasa Kataoka, Takashi Tsukagoshi
Summary: High-resolution ALMA dust continuum observations towards a compact disk around CW Tau reveal different spectral slopes at various bands. Parametric fitting suggests that the CW Tau disk may be marginally gravitationally unstable. The total dust mass estimation and gap structure detection provide valuable insights into the disk's characteristics.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Evan A. Rich, John D. Monnier, Alicia Aarnio, Anna S. E. Laws, Benjamin R. Setterholm, David J. Wilner, Nuria Calvet, Tim Harries, Chris Miller, Claire L. Davies, Fred C. Adams, Sean M. Andrews, Jaehan Bae, Catherine Espaillat, Alexandra Z. Greenbaum, Sasha Hinkley, Stefan Kraus, Lee Hartmann, Andrea Isella, Melissa McClure, Rebecca Oppenheimer, Laura M. Perez, Zhaohuan Zhu
Summary: We present a complete sample of protoplanetary disks, searching for signatures of disk evolution and ongoing planet formation. Our findings show that the presence of a companion significantly reduces polarized flux levels, far-IR excess correlates with polarized flux for nonbinary systems, and systems with ring structures have low stellar masses. Additionally, we discovered several extremely young FS CMa systems.
ASTRONOMICAL JOURNAL
(2022)
Correction
Astronomy & Astrophysics
Karin Oberg, L. Ilsedore Cleeves, Jennifer B. Bergner, Joseph Cavanaro, Richard Teague, Jane Huang, Ryan A. Loomis, Edwin A. Bergin, Geoffrey A. Blake, Jenny Calahan, Paolo Cazzoletti, Viviana Veloso Guzman, Michiel R. Hogerheijde, Mihkel Kama, Jeroen Terwisscha van Scheltinga, Chunhua Qi, Ewine van Dishoeck, Catherine Walsh, David J. Wilner
ASTRONOMICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Devin Sullivan, David J. Wilner, Luca Matra, Mark C. Wyatt, Sean M. Andrews, Meredith A. MacGregor, Brenda Matthews
Summary: The millimeter observations of the Pleiades star cluster using ALMA provide consistent results with steady-state collisional cascade model, indicating no abnormal collisions beyond the predictions of the model.
ASTRONOMICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Richard Teague, Jaehan Bae, Sean M. Andrews, Myriam Benisty, Edwin A. Bergin, Stefano Facchini, Jane Huang, Cristiano Longarini, David Wilner
Summary: We present ALMA observations of the CO J = 2 - 1 and CS J = 5 - 4 emission from the disk around TW Hydrae, which shows a predominantly Keplerian velocity structure. The rotation velocity slows down at the outer edge of the disk due to enhanced pressure support from the gas density taper. Localized deviations in the gas kinematics traced by CO and CS are revealed, and both molecules exhibit a Doppler flip feature centered along the minor axis of the disk. The features are interpreted as interactions with a Saturn-mass planet within the observed gap, consistent with theoretical predictions.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
David Vizgan, A. Meredith Hughes, Evan S. Carter, Kevin M. Flaherty, Margaret Pan, Eugene Chiang, Hilke Schlichting, David J. Wilner, Sean M. Andrews, John M. Carpenter, Attila Moor, Meredith A. MacGregor
Summary: Debris disks, which are scaled-up analogs of the Kuiper Belt, generate dust through collisions between planetesimals. By observing the debris disk around the nearby M dwarf AU Microscopii, researchers discovered that smaller bodies are more easily disrupted by collisions, contradicting current assumptions.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Ward S. Howard, Meredith A. MacGregor, Rachel Osten, Jan Forbrich, Steven R. Cranmer, Isaiah Tristan, Alycia J. Weinberger, Allison Youngblood, Thomas Barclay, R. O. Parke Loyd, Evgenya L. Shkolnik, Andrew Zic, David J. Wilner
Summary: This paper presents millimeter, optical, and soft X-ray observations of a stellar flare with an energy comparable to typical X1 solar flares. The study finds that millimeter emission appears to be common in small stellar flares, which had gone undetected until recently, making it challenging to interpret these events within the current multi-wavelength picture of flaring processes. The smallest stellar millimeter flare detected to date is reported, and the relationship between soft X-ray and millimeter emission is compared to that observed in solar flares.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Tomohiro C. Yoshida, Hideko Nomura, Takashi Tsukagoshi, Kenji Furuya, Takahiro Ueda
Summary: Using archival data from the Atacama Large Millimeter/submillimeter Array (ALMA), researchers have directly determined the gas surface density of a protoplanetary disk for the first time. The study revealed that the inner region of the disk has enough mass to form a Jupiter-mass planet and identified a significant drop in gas surface density at the inner cavity compared to outside the cavity.
ASTROPHYSICAL JOURNAL LETTERS
(2022)
Article
Astronomy & Astrophysics
Jesse Bublitz, Joel H. Kastner, Pierre Hily-Blant, Thierry Forveille, Miguel Santander-Garcia, Javier Alcolea, Valentin Bujarrabal, David J. Wilner, Rodolfo Montez, Isabel Aleman
Summary: Observations of CO+ and HCO+ in the young planetary nebula NGC 7027 reveal that UV radiation from the central star drives CO+ formation, while dust-penetrating soft X-rays enhance the abundance of HCO+ in the surrounding molecular envelope, forming an X-ray dominated region (XDR). These observations clearly demonstrate the influence of stellar irradiation on molecular gas formation.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Carlos E. Munoz-Romero, Karin I. Oberg, Charles J. Law, Richard Teague, Yuri Aikawa, Jennifer B. Bergner, David J. Wilner, Jane Huang, Viviana V. Guzman, L. Ilsedore Cleeves
Summary: Through new observations and archival data, researchers have found similar disk-averaged column densities and kinetic temperatures for DCO+ and DCN in the protoplanetary disk around TW Hya, indicating a common origin near the comet- and planet-forming midplane. The observed DCO+/DCN abundance ratio, combined with modeling results, provide tentative evidence of a gas-phase C/O enhancement within <40 au. Observations of DCO+ and DCN in other disks, as well as HCN and HCO+, will be necessary to fully understand the deuteration mechanisms in disks.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Shinji Fujita, Atsushi M. Ito, Yusuke Miyamoto, Yasutomo Kawanishi, Kazufumi Torii, Yoshito Shimajiri, Atsushi Nishimura, Kazuki Tokuda, Toshikazu Ohnishi, Hiroyuki Kaneko, Tsuyoshi Inoue, Shunya Takekawa, Mikito Kohno, Shota Ueda, Shimpei Nishimoto, Ryuki Yoneda, Kaoru Nishikawa, Daisuke Yoshida
Summary: This study attempts to use a convolutional neural network (CNN) to construct a two-class model for determining the distance to molecular clouds in the Galaxy, with a 76% accuracy rate on the training dataset.
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
(2023)
Review
Astronomy & Astrophysics
Kamber R. Schwarz, Joan Najita, Jennifer Bergner, John Carr, Alexander Tielens, Edwin A. Bergin, David Wilner, David Leisawitz, Christopher K. Walker
Summary: The NASA mission concept OASIS aims to track the journey of water from galaxies to protostellar systems to Earth's oceans. This paper focuses on the achievable science of protoplanetary disks with OASIS's heterodyne receivers, allowing for high-resolution observations of water vapor and HD isotopologue, which provide insights into the spatial distribution and evolutionary stages of water in disks and its role in planet formation.
SPACE SCIENCE REVIEWS
(2023)