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86 papers
Cold molecular gas in the hot nuclear wind of the Milky Way
M. Heyer, E. Di Teodoro, L. Loinard +3
Using the Large Millimeter Telescope and the SEQUOIA 3~mm focal plane array, we have searched for molecular line emission from two atomic clouds associated with the Fermi Bubble of…
Limits on the OH Molecule in the Smith High Velocity Cloud
Anthony H. Minter, Felix J. Lockman, S. A. Balashev +1
We have used the Green Bank Telescope (GBT) to search for the OH molecule at several locations in the Smith Cloud, one of the most prominent of the high-velocity clouds that surrou…
The Metallicities of Five Small High-Velocity Clouds
Trisha Ashley, Andrew J. Fox, Felix J. Lockman +5
High-velocity clouds (HVCs) are multi-phase gas structures whose velocities (|v_LSR|>100 km/s) are too high to be explained by Galactic disk rotation. While large HVCs are well cha…
Direct observations of the atomic-molecular phase transition in the Milky Way's nuclear wind
Karlie A. Noon, Mark R. Krumholz, Enrico M. Di Teodoro +3
Hundreds of high-velocity atomic gas clouds exist above and below the Galactic Centre, with some containing a molecular component. However, the origin of these clouds in the Milky…
A Component of the Smith High Velocity Cloud Now Crossing the Galactic Plane
Felix J. Lockman, Robert A. Benjamin, Nicolas Pichette +1
We have identified a new structure in the Milky Way: a leading component of the Smith high velocity cloud that is now crossing the Galactic plane near longitude 25 degrees. Using n…
Diverse metallicities of Fermi bubble clouds indicate dual origins in the disk and halo
Trisha Ashley, Andrew J. Fox, Frances H. Cashman +5
The Galactic Center is surrounded by two giant plasma lobes known as the Fermi Bubbles, extending ~10 kpc both above and below the Galactic plane. Spectroscopic observations of Fer…