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Browsing by Author "Andersson, B. -G"

Browsing by Author "Andersson, B. -G"

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  • Charting the Interstellar Magnetic Field causing the Interstellar Boundary Explorer (IBEX) Ribbon of Energetic Neutral Atoms 
    Frisch, P. C.; Berdyugin, A.; Piirola, V.; Magalhaes, A. M.; Seriacopi, D. B.; Wiktorowicz, S. J.; Andersson, B. -G; Funsten, H. O.; McComas, D. J.; Schwadron, N. A.; Slavin, Jonathan D.; Hanson, A. J.; Fu, C. -W (2015)
    The interstellar magnetic field (ISMF) near the heliosphere is a fundamental component of the solar galactic environment that can only be studied using polarized starlight. The results of an ongoing survey of the linear ...
  • Comparisons of the Interstellar Magnetic Field Directions Obtained from the IBEX Ribbon and Interstellar Polarizations 
    Frisch, Priscilla C.; Andersson, B. -G; Berdyugin, Andrei; Funsten, Herbert O.; Magalhaes, Antonio M.; McComas, David J.; Piirola, Vilppu; Schwadron, Nathan A.; Slavin, Jonathan D.; Wiktorowicz, Sloane J. (2010)
    Variations in the spatial configuration of the interstellar magnetic field (ISMF) near the Sun can be constrained by comparing the ISMF direction at the heliosphere found from the Interstellar Boundary Explorer (IBEX) ...
  • Evidence for an Interstellar Dust Filament in the Outer Heliosheath 
    Frisch, P. C.; Andersson, B. -G; Berdyugin, A.; Piirola, V.; Funsten, H. O.; Magalhaes, A. M.; Seriacopi, D. B.; McComas, D. J.; Schwadron, N. A.; Slavin, Jonathan D.; Wiktorowicz, S. J. (2015)
    A recently discovered filament of polarized starlight that traces a coherent magnetic field is shown to have several properties that are consistent with an origin in the outer heliosheath of the heliosphere: (1) the magnetic ...
  • HAWC+/SOFIA Multiwavelength Polarimetric Observations of OMC-1 
    Chuss, David T.; Andersson, B. -G; Bally, John; Dotson, Jessie L.; Dowell, C. Darren; Guerra, Jordan A.; Harper, Doyal A.; Houde, Martin; Jones, Terry Jay; Lazarian, A.; Lopez Rodriguez, Enrique; Michail, Joseph M.; Morris, Mark R.; Novak, Giles; Siah, Javad; Staguhn, Johannes; Vaillancourt, John E.; Volpert, C. G.; Werner, Michael; Wollack, Edward J.; Benford, Dominic J.; Berthoud, Marc; Cox, Erin G.; Crutcher, Richard; Dale, Daniel A.; Fissel, L. M.; Goldsmith, Paul F.; Hamilton, Ryan T.; Hanany, Shaul; Henning, Thomas K.; Looney, Leslie W.; Moseley, S. Harvey; Santos, Fabio P.; Stephens, Ian; Tassis, Konstantinos; Trinh, Christopher Q.; Van Camp, Eric; Ward-Thompson, Derek; HAWC + Science Team (2019)
    We report new polarimetric and photometric maps of the massive star-forming region OMC-1 using the HAWC+ instrument on the Stratospheric Observatory for Infrared Astronomy. We present continuum polarimetric and photometric ...
  • The Interstellar Magnetic Field Close to the Sun. II. 
    Frisch, P. C.; Andersson, B. -G; Berdyugin, A.; Piirola, V.; DeMajistre, R.; Funsten, H. O.; Magalhaes, A. M.; Seriacopi, D. B.; McComas, D. J.; Schwadron, N. A.; Slavin, Jonathan D.; Wiktorowicz, S. J. (2012)
    The magnetic field in the local interstellar medium (ISM) provides a key indicator of the galactic environment of the Sun and influences the shape of the heliosphere. We have studied the interstellar magnetic field (ISMF) ...
  • The Magnetic Field in the Milky Way Filamentary Bone G47 
    Stephens, Ian W.; Myers, Philip C.; Zucker, Catherine; Jackson, James M.; Andersson, B. -G; Smith, Rowan; Soam, Archana; Battersby, Cara; Sanhueza, Patricio; Hogge, Taylor; Smith, Howard A.; Novak, Giles; Sadavoy, Sarah; Pillai, Thushara G. S.; Li, Zhi-Yun; Looney, Leslie W.; Sugitani, Koji; Coudé, Simon; Guzmán, Andrés; Goodman, Alyssa; Kusune, Takayoshi; Santos, Fábio P.; Zuckerman, Leah; Encalada, Frankie (2022)
    Star formation primarily occurs in filaments where magnetic fields are expected to be dynamically important. The largest and densest filaments trace the spiral structure within galaxies. Over a dozen of these dense ...
  • Magnetic Fields in the Infrared Dark Cloud G34.43+0.24 
    Soam, Archana; Liu, Tie; Andersson, B. -G; Lee, Chang Won; Liu, Junhao; Juvela, Mika; Li, Pak Shing; Goldsmith, Paul F.; Zhang, Qizhou; Koch, Patrick M.; Kim, Kee-Tae; Qiu, Keping; Evans, Neal J., II; Johnstone, Doug; Thompson, Mark; Ward-Thompson, Derek; Di Francesco, James; Tang, Ya-Wen; Montillaud, Julien; Kim, Gwanjeong; Mairs, Steve; Sanhueza, Patricio; Kim, Shinyoung; Berry, David; Gordon, Michael S.; Tatematsu, Ken'ichi; Liu, Sheng-Yuan; Pattle, Kate; Eden, David; McGehee, Peregrine M.; Wang, Ke; Ristorcelli, I.; Graves, Sarah F.; Alina, Dana; Lacaille, Kevin M.; Montier, Ludovic; Park, Geumsook; Kwon, Woojin; Chung, Eun Jung; Pelkonen, Veli-Matti; Micelotta, Elisabetta R.; Saajasto, Mika; Fuller, Gary (2019)
    We present the B-fields mapped in IRDC G34.43+0.24 using 850 µm polarized dust emission observed with the POL-2 instrument at the James Clerk Maxwell telescope. We examine the magnetic field geometries and strengths in the ...
  • SOFIA Observations of 30 Doradus. II. Magnetic Fields and Large-scale Gas Kinematics 
    Tram, Le Ngoc; Bonne, Lars; Hu, Yue; Lopez-Rodriguez, Enrique; Guerra, Jordan A.; Lesaffre, Pierre; Gusdorf, Antoine; Hoang, Thiem; Lee, Min-Young; Lazarian, Alex; Andersson, B. -G; Coudé, Simon; Soam, Archana; Vacca, William D.; Lee, Hyeseung; Gordon, Michael (2023)
    The heart of the Large Magellanic Cloud, 30 Doradus, is a complex region with a clear core-halo structure. Feedback from the stellar cluster R136 has been shown to be the main source of energy creating multiple parsec-scale ...

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