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  • Butzer, Karl W.; Helgren, David M.; Fock, G. J.; Stuckenrath, Robert, Jr. (1973)
  • Wu, Ya-Lin; Bowler, Brendan P.; Sheehan, Patrick D.; Andrews, Sean M.; Herczeg, Gregory J.; Kraus, Adam L.; Ricci, Luca; Wilner, David J.; Zhu, Zhaohuan (2020)
    Characterizing the physical properties and compositions of circumplanetary disks can provide important insights into the formation of giant planets and satellites. We report Atacama Large Millimeter/submillimeter Array ...
  • Sullivan, Devin; Wilner, David J.; Matrà, Luca; Wyatt, Mark C.; Andrews, Sean M.; MacGregor, Meredith A.; Matthews, Brenda (2022)
    Millimeter emission from debris disks around stars of different ages provides constraints on the collisional evolution of planetesimals. We present ALMA 1.3 millimeter observations of a sample of 76 Solar-type stars in the ...
  • Su, Kate Y. L.; MacGregor, Meredith A.; Booth, Mark; Wilner, David J.; Flaherty, Kevin; Hughes, A. Meredith; Phillips, Neil M.; Malhotra, Renu; Hales, Antonio S.; Morrison, Sarah; Ertel, Steve; Matthews, Brenda C.; Dent, William R. F.; Casassus, Simon (2017)
    Planets and minor bodies such as asteroids, Kuiper-Belt objects, and comets are integral components of a planetary system. Interactions among them leave clues about the formation process of a planetary system. The signature ...
  • White, Jacob Aaron; Kóspál, Á.; Hughes, A. G.; Ábrahám, P.; Akimkin, V.; Banzatti, A.; Chen, L.; Cruz-Sáenz de Miera, F.; Dutrey, A.; Flock, M.; Guilloteau, S.; Hales, A. S.; Henning, T.; Kadam, K.; Semenov, D.; Sicilia-Aguilar, A.; Teague, Richard D.; Vorobyov, E. I. (2020)
    Extreme outbursts in young stars may be a common stage of pre-main-sequence stellar evolution. These outbursts, caused by enhanced accretion and accompanied by increased luminosity, can also strongly impact the evolution ...
  • White, Jacob Aaron; Boley, A. C.; MacGregor, M. A.; Hughes, A. M.; Wilner, D. J. (2018)
    We present VLA 9 mm (33 GHz) and archival ALMA 2.9 mm (103 GHz) observations of the HD 141569 system. The VLA observations achieve a resolution of 0.25 arcsec (˜28 au) and a sensitivity of 4.7 µJy beam<SUP>- 1</SUP>. We ...
  • Loinard, Laurent; Zapata, Luis A.; Rodríguez, Luis F.; Pech, Gerardo; Chandler, Claire J.; Brogan, Crystal L.; Wilner, David J.; Ho, Paul T. P.; Parise, Bérengère; Hartmann, Lee W.; Zhu, Zhaohuan; Takahashi, Satoko; Trejo, Alfonso (2013)
    We present Atacama Large Millimeter/submillimeter Array (ALMA) and Very Large Array (VLA) observations of the molecular and ionized gas at 0.1-0.3 arcsec resolution in the Class 0 protostellar system IRAS 16293-2422. These ...
  • Garufi, A.; Podio, L.; Codella, C.; Rygl, K.; Bacciotti, F.; Facchini, S.; Fedele, D.; Miotello, A.; Teague, Richard; Testi, L. (2020)
    The chemical composition of planets is determined by the distribution of the various molecular species in the protoplanetary disk at the time of their formation. To date, only a handful of disks have been imaged in multiple ...
  • Podio, L.; Garufi, A.; Codella, C.; Fedele, D.; Rygl, K.; Favre, C.; Bacciotti, F.; Bianchi, E.; Ceccarelli, C.; Mercimek, S.; Teague, Richard D.; Testi, L. (2020)
    Context. Planets form in protoplanetary disks and inherit their chemical composition. It is therefore crucial to understand the molecular content of protoplanetary disks in their gaseous and solid components. <br/> Aims: ...
  • Garufi, A.; Podio, L.; Codella, C.; Fedele, D.; Bianchi, E.; Favre, C.; Bacciotti, F.; Ceccarelli, C.; Mercimek, S.; Rygl, K.; Teague, Richard; Testi, L. (2021)
    We present an overview of the ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT), a campaign devoted to the characterization of the molecular emission from partly embedded young stars. The project is aimed ...
  • Harrison, Rachel E.; Looney, Leslie W.; Stephens, Ian W.; Li, Zhi-Yun; Teague, Richard; Crutcher, Richard M.; Yang, Haifeng; Cox, Erin G.; Fernández-López, Manuel; Shinnaga, Hiroko (2021)
    While magnetic fields likely play an important role in driving the evolution of protoplanetary disks through angular momentum transport, observational evidence of magnetic fields has only been found in a small number of ...
  • Sano, Hidetoshi; Tsuge, Kisetsu; Tokuda, Kazuki; Muraoka, Kazuyuki; Tachihara, Kengo; Yamane, Yumiko; Kohno, Mikito; Fujita, Shinji; Enokiya, Rei; Rowell, Gavin; Maxted, Nigel; Filipovic, Miroslav D.; Knies, Jonathan; Sasaki, Manami; Onishi, Toshikazu; Plucinsky, Paul P.; Fukui, Yasuo (2021)
    We report the first evidence for high-mass star formation triggered by collisions of molecular clouds in M 33. Using the Atacama Large Millimeter/submillimeter Array, we spatially resolved filamentary structures of giant ...
  • Sano, H.; Plucinsky, Paul P.; Bamba, A.; Sharda, P.; Filipovic, M. D.; Law, Charles J.; Alsaberi, R. Z. E.; Yamane, Y.; Tokuda, K.; Acero, F.; Sasaki, M.; Vink, J.; Inoue, T.; Inutsuka, S.; Shimoda, J.; Tsuge, K.; Fujii, K.; Voisin, F.; Maxted, N.; Rowell, G.; Onishi, T.; Kawamura, A.; Mizuno, N.; Yamamoto, H.; Tachihara, K.; Fukui, Y. (2020)
    N132D is the brightest gamma-ray supernova remnant (SNR) in the Large Magellanic Cloud (LMC). We carried out <SUP>12</SUP>CO(J = 1-0, 3-2) observations toward the SNR using the Atacama Large Millimeter/submillimeter Array ...
  • Consiglio, S. Michelle; Turner, Jean L.; Beck, Sara; Meier, David S.; Silich, Sergiy; Zhao, Jun-Hui (2017)
    We report ALMA observations of <SUP>12</SUP>CO(3-2) and <SUP>13</SUP>CO(3-2) in the gas-poor dwarf galaxy NGC 5253. These 0.´´3(5.5 pc) resolution images reveal small, dense molecular gas clouds that are located in ...
  • Bowler, Brendan P.; Andrews, Sean M.; Kraus, Adam L.; Ireland, Michael J.; Herczeg, Gregory; Ricci, Luca; Carpenter, John; Brown, Michael E. (2015)
    We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of GSC 6214-210 A and B, a solar-mass member of the 5–10 Myr Upper Scorpius association with a 15 ± 2 M<SUB>Jup</SUB> companion orbiting at ˜ 330 ...
  • Decin, L.; Richards, A. M. S.; Neufeld, D.; Steffen, W.; Melnick, G.; Lombaert, R. (2015)
    Context. Evolved low-mass stars lose a significant fraction of their mass through stellar winds. While the overall morphology of the stellar wind structure during the asymptotic giant branch (AGB) phase is thought to be ...
  • MacGregor, Meredith A.; Weinberger, Alycia J.; Hughes, A. Meredith; Wilner, David J.; Currie, Thayne; Debes, John H.; Donaldson, Jessica K.; Redfield, Seth; Roberge, Aki; Schneider, Glenn (2018)
    We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm (230 GHz) observations of the HD 32297 and HD 61005 debris disks, two of the most iconic debris disks because of their dramatic swept-back wings seen ...
  • Xue, Ci; Remijan, Anthony J.; Brogan, Crystal L.; Hunter, Todd R.; Herbst, Eric; McGuire, Brett A. (2019)
    Vibrationally excited states of detected interstellar molecules have been shown to account for a large portion of unidentified spectral lines in observed interstellar spectra toward chemically rich sources. Here, we present ...
  • Turner, Jean L.; Consiglio, S. Michelle; Beck, Sara C.; Goss, W. M.; Ho, Paul T. P.; Meier, David S.; Silich, Sergiy; Zhao, Jun-Hui (2017)
    We present observations of CO(3-2) and <SUP>13</SUP>CO(3-2) emission near the supernebula in the dwarf galaxy NGC 5253, which contains one of the best examples of a potential globular cluster in formation. The 0.´´3 ...
  • Nagai, H.; Onishi, K.; Kawakatu, N.; Fujita, Y.; Kino, M.; Fukazawa, Y.; Lim, J.; Forman, William; Vrtilek, Jan; Nakanishi, K.; Noda, H.; Asada, K.; Wajima, K.; Ohyama, Y.; David, Laurence; Daikuhara, K. (2019)
    We present observations using the Atacama Large Millimeter/submillimeter Array of the CO(2-1), HCN(3-2), and HCO<SUP>+</SUP>(3-2) lines in the nearby radio galaxy/brightest cluster galaxy (BCG) NGC 1275 with a spatial ...

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