By Elizabeth Tarantino and Joan Schmelz
Paper: Characterizing the Multiphase Origin of [C II] Emission in M101 and NGC 6946 with Velocity-resolved Spectroscopy
Tarantino, Elizabeth, et al., 2021/07, ApJ, 915, 92.
By Enrique Lopez-Rodriguez and Joan Schmelz
Paper: Extragalactic Magnetism with SOFIA (Legacy Program) - II: A Magnetically Driven Flow in the Starburst Ring of NGC 1097
Lopez-Rodriguez, Enrique, et al., 2021/12, ApJ, 923, 150.
Magnetically-driven flows feed the super massive blackhole at the center of NGC 1097. SOFIA investigated this long-standing problem of the large-scale transfer of matter from the body of the host galaxy to the active nucleus.
By Dario Fadda and Joan Schmelz
Paper: [C II] and CO Emission along the Bar and Counter-arms of NGC 7479
Fadda, Dario, et al., 2021/03, ApJ, 909, 204.
SOFIA observations of the barred spiral galaxy, NGC 7479, were able to separate shock-enhanced ionized carbon [CII] emission from that associated with star formation, reminding us that it is important to consider multiple mechanisms when studying the [CII] emission in galaxies with active nuclei.
By Alejandro Borlaff and Joan Schmelz
Paper: Extragalactic Magnetism with SOFIA (Legacy Program). I. The Magnetic Field in the Multiphase Interstellar Medium of M51
Alejandro S. Borlaff et al 2021 ApJ 921 128
By Enrique Lopez Rodrigues & Joan Schmelz
Paper: The Magnetic Field Across the Molecular Warped Disk of Centaurus A
Lopez-Rodriguez, E., Nat Astron (2021).
By Joan Schmelz
Paper: The Strength and Structure of the Magnetic Field in the Galactic Outflow of Messier 82
Lopez-Rodriguez, E., et al., 2021 ApJ 914 24
By Kevin Cooke, Allison Kirkpatrick, and Joan Schmelz
Paper: Dying of the Light: An X-Ray Fading Cold Quasar at z ~ 0.405
Cooke, K. C. et al., 2020 ApJ 903 106
By Enrique Lopez-Rodriguez and Joan Schmelz
Paper: SOFIA/HAWC+ Traces the Magnetic Felds in NGC 1068
Lopez-Rodriguez et al., 2020, ApJ, 888, 66.
SOFIA astronomers have measured, for the first time, the magnetic field tracing the star forming regions along the spiral arms of NGC 1068, the nearest grand-design spiral with an active galactic nuclei and a large-scale almost face-on disk.
By Joan Schmelz
How do astronomers understand galaxies that are so far away that they may appear as a simple point source, even when observed with the most powerful telescopes? One proven technique is to study local analogues, galaxies that might have similar properties but are close enough to resolve their structures. A study like this was underway when researchers discovered something extraordinary – their observation was 10 times stronger than predicted.
By Terry Jones, Arielle Moullet, Kassandra Bell, and Joan Schmelz
Paper: SOFIA Far Infrared Imaging Polarimetry of M82 and NGC 253: Exploring the Super–Galactic Wind
Jones, Terry Jay, et al., 2019, ApJL, 870, L9.