Article
Astronomy & Astrophysics
Charles J. Law, Ryan A. Loomis, Richard Teague, Karin Oberg, Ian Czekala, Sean M. Andrews, Jane Huang, Yuri Aikawa, Felipe Alarcon, Jaehan Bae, Edwin A. Bergin, Jennifer B. Bergner, Yann Boehler, Alice S. Booth, Arthur D. Bosman, Jenny K. Calahan, Gianni Cataldi, L. Ilsedore Cleeves, Kenji Furuya, Viviana V. Guzman, John D. Ilee, Romane Le Gal, Yao Liu, Feng Long, Francois Menard, Hideko Nomura, Chunhua Qi, Kamber R. Schwarz, Anibal Sierra, Takashi Tsukagoshi, Yoshihide Yamato, Merel L. R. van't Hoff, Catherine Walsh, David J. Wilner, Ke Zhang
Summary: The study reveals the existence of a large number of different chemical substructures in protoplanetary disks, which can be found at different radii. Most of these chemical substructures coincide spatially with dust substructures in the inner regions of the disks, while some cannot be directly linked to dust substructures. This suggests that chemical substructures could represent different disk characteristics and influence the environment in which planets assemble.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Yuri Aikawa, Gianni Cataldi, Yoshihide Yamato, Ke Zhang, Alice S. Booth, Kenji Furuya, Sean M. Andrews, Jaehan Bae, Edwin A. Bergin, Jennifer B. Bergner, Arthur D. Bosman, L. Ilsedore Cleeves, Ian Czekala, Viviana V. Guzman, Jane Huang, John D. Ilee, Charles J. Law, Romane Le Gal, Ryan A. Loomis, Francois Menard, Hideko Nomura, Karin Oberg, Chunhua Qi, Kamber R. Schwarz, Richard Teague, Takashi Tsukagoshi, Catherine Walsh, David J. Wilner
Summary: The study observed the distribution and abundance of HCO+ and (HCO+)-C-13 molecular ions in five protoplanetary disks, revealing specific features in different radius ranges and showing differences in ionization degree in key regions inside and outside the disks, which are consistent with the template disk model.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Maria Galloway-Sprietsma, Jaehan Bae, Richard Teague, Myriam Benisty, Stefano Facchini, Yuri Aikawa, Felipe Alarcon, Sean M. Andrews, Edwin Bergin, Gianni Cataldi, L. Ilsedore Cleeves, Ian Czekala, Viviana V. Guzman, Jane Huang, Charles J. Law, Romane Le Gal, Yao Liu, Feng Long, Francois Menard, Karin I. Oberg, Catherine Walsh, David J. Wilner
Summary: We studied the kinematics of the AS 209 disk by analyzing the transitions of (CO)-C-12, (CO)-C-13, and (CO)-O-18. We found an upward flow of gas originating from the annular gap, which is difficult to explain with an embedded planet alone. Instead, we propose that magnetically driven winds triggered by low gas density within the gap dominate the kinematics of the region. The activation of these winds may control the growth of the embedded planet and explain the scarcity of directly imaged super-Jovian-mass planets.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Arthur D. Bosman, Edwin A. Bergin, Ryan A. Loomis, Sean M. Andrews, Merel L. R. Van't Hoff, Richard Teague, Karin Oberg, Viviana V. Guzman, Catherine Walsh, Yuri Aikawa, Felipe Alarcon, Jaehan Bae, Jennifer B. Bergner, Alice S. Booth, Gianni Cataldi, L. Ilsedore Cleeves, Ian Czekala, Jane Huang, John D. Ilee, Charles J. Law, Romane Le Gal, Yao Liu, Feng Long, Francois Menard, Hideko Nomura, Laura M. Perez, Chunhua Qi, Kamber R. Schwarz, Anibal Sierra, Takashi Tsukagoshi, Yoshihide Yamato, David J. Wilner, Ke Zhang
Summary: Constraining the distribution of gas and dust in the inner regions of protoplanetary disks is challenging, but using the sensitivity of the ALMA MAPS program can reveal important relationships between gas and dust. Observations of IM Lup, GM Aur, AS 209, and HD 163296 disks show different patterns of gas and dust distribution, providing insights into key processes in planet formation.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Richard Teague, Jaehan Bae, Yuri Aikawa, Sean M. Andrews, Edwin A. Bergin, Jennifer B. Bergner, Yann Boehler, Alice S. Booth, Arthur D. Bosman, Gianni Cataldi, Ian Czekala, Viviana V. Guzman, Jane Huang, John D. Ilee, Charles J. Law, Romane Le Gal, Feng Long, Ryan A. Loomis, Francois Menard, Karin Oberg, Laura M. Perez, Kamber R. Schwarz, Anibal Sierra, Catherine Walsh, David J. Wilner, Yoshihide Yamato, Ke Zhang
Summary: The study investigates the dynamical structure of protoplanetary disks around HD 163296 and MWC 480, revealing perturbations and tightly wound spiral arms that suggest the presence of embedded giant planets. The findings demonstrate the potential of molecular line observations in characterizing disk dynamics and searching for planetary signatures.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Jaehan Bae, Richard Teague, Sean M. Andrews, Myriam Benisty, Stefano Facchini, Maria Galloway-Sprietsma, Ryan A. Loomis, Yuri Aikawa, Felipe Alarcon, Edwin Bergin, Jennifer B. Bergner, Alice S. Booth, Gianni Cataldi, L. Ilsedore Cleeves, Ian Czekala, Viviana V. Guzman, Jane Huang, John D. Ilee, Nicolas T. Kurtovic, Charles J. Law, Romane Le Gal, Yao Liu, Feng Long, Francois Menard, Karin Oberg, Laura M. Perez, Chunhua Qi, Kamber R. Schwarz, Anibal Sierra, Catherine Walsh, David J. Wilner, Ke Zhang
Summary: This paper reports the discovery of a candidate circumplanetary disk (CPD) in the circumstellar disk of the T Tauri star AS 209. This is the first instance of CPD detection using gaseous emission, which allows for tracing of the CPD mass. The CPD has a high gas temperature and a low dust-to-gas mass ratio.
ASTROPHYSICAL JOURNAL LETTERS
(2022)
Article
Astronomy & Astrophysics
Jennifer B. Bergner, Karin I. Oberg, Viviana V. Guzman, Charles J. Law, Ryan A. Loomis, Gianni Cataldi, Arthur D. Bosman, Yuri Aikawa, Sean M. Andrews, Edwin A. Bergin, Alice S. Booth, L. Ilsedore Cleeves, Ian Czekala, Jane Huang, John D. Ilee, Romane Le Gal, Feng Long, Hideko Nomura, Francois Menard, Chunhua Qi, Kamber R. Schwarz, Richard Teague, Takashi Tsukagoshi, Catherine Walsh, David J. Wilner, Yoshihide Yamato
Summary: UV photochemistry alters the composition of protoplanetary disk surface layers significantly, with CN/HCN ratio increasing with disk radius. Millimeter dust gaps and rings impact the CN/HCN ratio, indicating CN is the main carrier and different disk layers are chemically linked.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Jenny K. Calahan, Edwin A. Bergin, Ke Zhang, Kamber R. Schwarz, Karin Oberg, Viviana V. Guzman, Catherine Walsh, Yuri Aikawa, Felipe Alarcon, Sean M. Andrews, Jaehan Bae, Jennifer B. Bergner, Alice S. Booth, Arthur D. Bosman, Gianni Cataldi, Ian Czekala, Jane Huang, John D. Ilee, Charles J. Law, Romane Le Gal, Feng Long, Ryan A. Loomis, Francois Menard, Hideko Nomura, Chunhua Qi, Richard Teague, Merel L. R. van't Hoff, David J. Wilner, Yoshihide Yamato
Summary: Understanding the temperature structure of protoplanetary disks is crucial for interpreting observations, predicting disk evolution, and modeling planet formation processes. This study constrains the thermal structure of the disk around HD 163296, reproducing high-resolution ALMA observations and indicating radial CO depletion and enhanced temperatures near the disk surface.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Ke Zhang, Alice S. Booth, Charles J. Law, Arthur D. Bosman, Kamber R. Schwarz, Edwin A. Bergin, Karin Oberg, Sean M. Andrews, Viviana V. Guzman, Catherine Walsh, Chunhua Qi, Merel L. R. van 't Hoff, Feng Long, David J. Wilner, Jane Huang, Ian Czekala, John D. Ilee, Gianni Cataldi, Jennifer B. Bergner, Yuri Aikawa, Richard Teague, Jaehan Bae, Ryan A. Loomis, Jenny K. Calahan, Felipe Alarcon, Francois Menard, Romane Le Gal, Anibal Sierra, Yoshihide Yamato, Hideko Nomura, Takashi Tsukagoshi, Laura M. Perez, Leon Trapman, Yao Liu, Kenji Furuya
Summary: High-resolution observations of CO isotopologue lines using ALMA Large Program revealed significant variations in CO gas column density profiles among five protoplanetary disks, with distributions matching well with viscous disk models. The study also found correlations between CO gas gaps and continuum gap locations, as well as depths of gaps consistent with predictions of planet-disk interactions.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Karin Oberg, Viviana V. Guzman, Catherine Walsh, Yuri Aikawa, Edwin A. Bergin, Charles J. Law, Ryan A. Loomis, Felipe Alarcon, Sean M. Andrews, Jaehan Bae, Jennifer B. Bergner, Yann Boehler, Alice S. Booth, Arthur D. Bosman, Jenny K. Calahan, Gianni Cataldi, L. Ilsedore Cleeves, Ian Czekala, Kenji Furuya, Jane Huang, John D. Ilee, Nicolas T. Kurtovic, Romane Le Gal, Yao Liu, Feng Long, Francois Menard, Hideko Nomura, Laura M. Perez, Chunhua Qi, Kamber R. Schwarz, Anibal Sierra, Richard Teague, Takashi Tsukagoshi, Yoshihide Yamato, Merel L. R. van't Hoff, Abygail R. Waggoner, David J. Wilner, Ke Zhang
Summary: The distribution of molecules in disks around young stars plays a crucial role in determining the elemental compositions of planets and their access to important compounds such as water and organics. Through ALMA observations, researchers have made significant discoveries about the links between dust, gas, and chemical substructures in these disks, reshaping our understanding of planet formation chemistry.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Kamber R. Schwarz, Jenny K. Calahan, Ke Zhang, Felipe Alarcon, Yuri Aikawa, Sean M. Andrews, Jaehan Bae, Edwin A. Bergin, Alice S. Booth, Arthur D. Bosman, Gianni Cataldi, L. Ilsedore Cleeves, Ian Czekala, Jane Huang, John D. Ilee, Charles J. Law, Romane Le Gal, Yao Liu, Feng Long, Ryan A. Loomis, Enrique Macias, Melissa McClure, Francois Menard, Karin I. Oberg, Richard Teague, Ewine van Dishoeck, Catherine Walsh, David J. Wilner
Summary: Gas mass in protoplanetary disks is challenging to constrain, but alternative tracers like dust, CO, and H-2 isotopologue HD can be used. By constructing a physical/chemical model, researchers found that the GM Aur protoplanetary disk is likely cold with a gas mass of approximately 0.2 M. However, a potentially unstable region between 70 and 100 AU was identified.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Jane Huang, Edwin A. Bergin, Karin Oberg, Sean M. Andrews, Richard Teague, Charles J. Law, Paul Kalas, Yuri Aikawa, Jaehan Bae, Jennifer B. Bergner, Alice S. Booth, Arthur D. Bosman, Jenny K. Calahan, Gianni Cataldi, L. Ilsedore Cleeves, Ian Czekala, John D. Ilee, Romane Le Gal, Viviana V. Guzman, Feng Long, Ryan A. Loomis, Francois Menard, Hideko Nomura, Chunhua Qi, Kamber R. Schwarz, Takashi Tsukagoshi, Merel L. R. van't Hoff, Catherine Walsh, David J. Wilner, Yoshihide Yamato, Ke Zhang
Summary: Research suggests that some protoplanetary disks interact with their surroundings, exhibiting complex gas structures and spiral arms, in contrast to the mostly axisymmetric, multi-ringed disks observed in millimeter continuum emission. These interactions may play a significant role in regulating material distribution and transport in the disk systems.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Charles J. Law, Richard Teague, Ryan A. Loomis, Jaehan Bae, Karin Oberg, Ian Czekala, Sean M. Andrews, Yuri Aikawa, Felipe Alarcon, Edwin A. Bergin, Jennifer B. Bergner, Alice S. Booth, Arthur D. Bosman, Jenny K. Calahan, Gianni Cataldi, L. Ilsedore Cleeves, Kenji Furuya, Viviana V. Guzman, Jane Huang, John D. Ilee, Romane Le Gal, Yao Liu, Feng Long, Francois Menard, Hideko Nomura, Laura M. Perez, Chunhua Qi, Kamber R. Schwarz, Daniela Soto, Takashi Tsukagoshi, Yoshihide Yamato, Merel L. R. van 't Hoff, Catherine Walsh, David J. Wilner, Ke Zhang
Summary: The ALMA's MAPS Large Program allows for the study of vertical distribution of gas, chemistry, and temperature in protoplanetary disks, with CO isotopes shown to trace the highest regions with emission height varying with radius.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
Article
Astronomy & Astrophysics
Haochang Jiang, Wei Zhu, Chris W. Ormel
Summary: Recently, a study investigated the correlation between line-emission and dust-continuum substructures, finding that the correlation is not universal. Outliers were also identified, particularly a strong correlation between chemical rings and dust gaps in MWC 480.
ASTROPHYSICAL JOURNAL LETTERS
(2022)
Article
Astronomy & Astrophysics
Viviana V. Guzman, Jennifer B. Bergner, Charles J. Law, Karin I. Oberg, Catherine Walsh, Gianni Cataldi, Yuri Aikawa, Edwin A. Bergin, Ian Czekala, Jane Huang, Sean M. Andrews, Ryan A. Loomis, Ke Zhang, Romane Le Gal, Felipe Alarcon, John D. Ilee, Richard Teague, L. Ilsedore Cleeves, David J. Wilner, Feng Long, Kamber R. Schwarz, Arthur D. Bosman, Laura M. Perez, Francois Menard, Yao Liu
Summary: The study reveals differences in column density and excitation temperature of HCN and C2H in protoplanetary disks, with HCN mainly present in a temperate layer and C2H in relatively warmer layers. The H2CO column densities are slightly higher in colder disks and increase near the CO snowline and/or millimeter dust edge, indicating efficient release of organic species in the outer disk.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2021)
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
Jane Huang, Edwin A. Bergin, Jaehan Bae, Myriam Benisty, Sean M. Andrews
Summary: DR Tau is known for its high variability compared to other T Tauri stars. Millimeter interferometry observations reveal the distribution of CO and other substances, showing the presence of a protoplanetary disk, gas envelope, asymmetrical outflow, and spiral arm with clumps. The CO arm is much larger than spiral arms seen in scattered light, highlighting the importance of sensitive molecular imaging for understanding the disk environment. Kinematics and compact emission distribution suggest that (CO)-O-18, SO, DCO+, and H2CO primarily originate from the circumstellar disk. The asymmetry in SO emission may be due to interaction with infalling material or unresolved substructure, indicating a complex environment similar to outbursting FUor and EXor sources, suggesting a link between DR Tau's extreme stellar activity and disk instabilities caused by large-scale infall.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Jamila Pegues, Karin Oberg, Chunhua Qi, Sean M. Andrews, Jane Huang, Charles J. Law, Romane Le Gal, Luca Matra, David J. Wilner
Summary: Protoplanetary disks around Herbig AeBe stars are exciting targets for studying the chemical environments where giant planets form. We conducted a pilot survey of millimeter continuum CO isotopologs and other small molecules in disks around five Herbig AeBe stars and detected or tentatively detected various molecular emissions. The flux ratios between CO 2-1 isotopologs were closest to unity for the Herbig AeBe/F disks, suggesting emitting layers with similar temperatures and more abundant CO relative to the disk dust mass. However, lower detection rates and flux ratios for certain molecules suggest smaller regimes of cold chemistry around the luminous Herbig AeBe/F stars.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
John Banovetz, Dan Milisavljevic, Niharika Sravan, Kathryn E. E. Weil, Bhagya Subrayan, Robert A. A. Fesen, Daniel J. J. Patnaude, Paul P. P. Plucinsky, Charles J. J. Law, William P. P. Blair, Jon A. A. Morse
Summary: In this study, proper motion measurements of the oxygen-rich ejecta of the LMC supernova remnant N132D were presented using data from the Hubble Space Telescope Advanced Camera for Surveys. The measurements revealed a center of expansion and an explosion age consistent with previous estimates. The proper motions of the ejecta were found to be ballistic and showed evidence of explosion asymmetry.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Charles J. J. Law, Richard Teague, Karin I. I. Oberg, Evan A. A. Rich, Sean M. M. Andrews, Jaehan Bae, Myriam Benisty, Stefano Facchini, Kevin Flaherty, Andrea Isella, Sheng Jin, Jun Hashimoto, Jane Huang, Ryan A. A. Loomis, Feng Long, Carlos E. E. Munoz-Romero, Teresa Paneque-Carreno, Laura M. M. Perez, Chunhua Qi, Kamber R. R. Schwarz, Jochen Stadler, Takashi Tsukagoshi, David J. J. Wilner, Gerrit van der Plas
Summary: High-spatial-resolution observations of CO isotopologue line emission in protoplanetary disks reveal detailed gas structure, including radial and vertical substructures, emission surface heights, and temperature profiles. Observations of CO, (CO)-C-13, and (CO)-O-18 in transition disks provide insights into disk structure and temperature distributions. The derived emission surfaces and temperature models show potential correlations with source characteristics, suggesting the influence of stellar host mass, gas temperature, and disk size on the emitting heights.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Juan Garrido-Deutelmoser, Cristobal Petrovich, Carolina Charalambous, Viviana V. Guzman, Ke Zhang
Summary: The ALMA observations of HD 163296 have discovered a crescent-shaped substructure inside a gap in the dust, which is caused by a compact pair of sub-Saturn-mass planets. This interpretation is supported by the gas gap measured from CO observations. Furthermore, a global model of the disk suggests that all four planets may form a long resonant chain.
ASTROPHYSICAL JOURNAL LETTERS
(2023)
Article
Astronomy & Astrophysics
Alessandra Canta, Karin I. Oberg, Mahesh Rajappan
Summary: This paper investigates the formation of CH3CN and related imines from the vacuum ultraviolet irradiation of NH3:C2H6, NH3:C2H4, and NH3:C2H2 ice mixtures. The results show that CH3CH=NH serves as an intermediate for the production of CH3CN, and its yield is generally higher than that of CH3CN. Furthermore, NH3:hydrocarbon ice photochemistry is proposed as an efficient formation pathway for low-temperature interstellar imines.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Shangjia Zhang, Matt Kalscheur, Feng Long, Ke Zhang, Deryl E. Long, Edwin A. Bergin, Zhaohuan Zhu, Leon Trapman
Summary: Observations of compact protoplanetary disks in the Taurus star-forming region reveal the presence of substructures at various radii. Comparison with other disk samples indicates that substructures are found in both small and large disks. Simulation results suggest that the occurrence rate of young planets peak at Neptune masses.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Abygail R. Waggoner, L. Ilsedore Cleeves, Ryan A. Loomis, Yuri Aikawa, Jaehan Bae, Jennifer B. Bergner, Alice S. Booth, Jenny K. Calahan, Gianni Cataldi, Charles J. Law, Romane Le Gal, Feng Long, Karin I. Oberg, Richard Teague, David J. Wilner
Summary: A study on the temporal flux variability of HCO(+)J = 1-0 in protoplanetary disks found variations in the spectral profiles, which may be attributed to variations in HCO+ flux and differences in uv coverage. These findings are consistent with the expectations of X-ray flare-driven chemistry.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Charles J. Law, Alice S. Booth, Karin I. oberg
Summary: Planets form in disks around young stars, altering the structure of the disk itself. The presence of planets can cause chemical asymmetries in the disk, detectable in gas observations. In the HD 169142 disk, there is evidence of a planet causing shocks and driving gas-phase SiS emission, as well as other chemical signatures related to planet formation. This disk serves as a template for future studies of planet-related chemical asymmetries.
ASTROPHYSICAL JOURNAL LETTERS
(2023)
Article
Astronomy & Astrophysics
Andrea Banzatti, Klaus M. Pontoppidan, John S. Carr, Evan Jellison, Ilaria Pascucci, Joan R. Najita, Carlos E. Munoz-Romero, Karin I. Oeberg, Anusha Kalyaan, Paola Pinilla, Sebastiaan Krijt, Feng Long, Michiel Lambrechts, Giovanni Rosotti, Gregory J. Herczeg, Colette Salyk, Ke Zhang, Edwin A. Bergin, Nicholas P. Ballering, Michael R. Meyer, Simon Bruderer
Summary: Previous analyses have found an anticorrelation between water luminosity and the millimeter dust disk radius in young protoplanetary disks. New observations using JWST-MIRI spectra reveal that compact disks have higher water emission compared to large disks, suggesting an enhanced inward mass flux of icy pebbles in compact disks. This opens up exciting prospects for studying planet formation chemistry with JWST.
ASTROPHYSICAL JOURNAL LETTERS
(2023)