HI Absorption Toward HII Regions at Small Galactic Longitudes
arXiv:1308.2769 · doi:10.1088/0004-637X/774/2/117
Abstract
We make a comprehensive study of HI absorption toward HII regions located within Galactic longitudes less than 10 degrees. Structures in the extreme inner Galaxy are traced using the longitude-velocity space distribution of this absorption. We find significant HI absorption associated with the Near and Far 3kpc Arms, the Connecting Arm, Banias Clump 1 and the H I Tilted Disk. We also constrain the line of sight distances to HII regions, by using HI absorption spectra together with the HII region velocities measured by radio recombination lines.
Complete figure set available in online version of journal. Accepted by ApJ August 8, 2013
References in corpus (10)
- Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
- Resolution of the Distance Ambiguity for Galactic HII Regions
- The Electron Temperature Gradient in the Galactic Disk
- Milky Way Kinematics: Measurements at the Subcentral Point of the Fourth Quadrant
- The Green Bank Telescope HII Region Discovery Survey: III. Kinematic Distances
- The Arecibo HII Region Discovery Survey
- Coupling the dynamics and the molecular chemistry in the Galactic center
- The large scale dust lanes of the Galactic bar
- High-Mass Star Formation in the Near and Far 3-KPC Arms
- Multiplicity of nuclear dust lanes and dust lane shocks in the Milky Way bar
Cited by in corpus (15)
- The observed spiral structure of the Milky Way
- ATLASGAL - Kinematic distances and the dense gas mass distribution of the inner Galaxy
- The SEDIGISM survey: first data release and overview of the Galactic structure
- A lack of classical Cepheids in the inner part of the Galactic disk
- First Parallax Measurements Towards a 6.7 GHz Methanol Maser with the Australian Long Baseline Array - Distance to G339.884-1.259
- The start of the Sagittarius spiral arm (Sagittarius origin) and the start of the Norma spiral arm (Norma origin) - model-computed and observed arm tangents at galactic longitudes -20 degrees < l < +23 degrees
- Timing the Milky Way bar formation and the accompanying radial migration episode
- SNR G349.7+0.2: A gamma-ray source in the far 3 kpc arm of the Galactic center
- HII Region Driven Galactic Bubbles and Their Relationship to the Galactic Magnetic Field
- Star formation in the Sh 2-53 region influenced by accreting molecular filaments
- A Complete Atlas of HI Absorption toward HII Regions in the Southern Galactic Plane Survey (SGPS1)
- New classical Cepheids in the inner part of the northern Galactic disk and their kinematics
- Surveying the Giant HII Regions of the Milky Way with SOFIA: IV. Sgr D, W42, and a Reassessment of the Giant HII Region Census
- Turbulent Pressure Heats Gas and Suppresses Star Formation in Galactic Bar Molecular Clouds
- Large-Scale Surveys of Pulsating Stars for Studying Stellar Populations in the Inner Galaxy