We present an HI absorption survey of the central 250 pc of the Galaxy. Very Large Array (VLA) observations were made at 21 cm in the DnC and CnB configurations and have a resolution of ∼15”(0.6 pc at the Galactic Center (GC) distance) and a velocity resolution of ∼2.5 km s−1. This study provides HI data with high spatial resolution, comparable with the many high resolution observations which have been made of GC sources over the past ten years. Here we present an overview of the HI absorption toward ∼40 well-known continuum sources and a detailed comparison of the ionized, atomic and molecular components of the interstellar medium for the Sgr B, Radio Arc and Sgr C regions. In these well-known regions, the atomic gas appears to be closely ...
Author Institution: Department of Astronomy and Astrophysics and Department of Chemistry, University...
Restricted Access.We present the highest resolution Very Large Array 74 MHz images of a ~ 10 degree ...
We present high-resolution (R = 20000) spectroscopy of H+3 absorption toward the luminous Galactic c...
We present an H I absorption survey of the central 250 pc of the Galaxy. Very Large Array observatio...
The neutral atomic gas content of galaxies is usually studied in the HI 21 cm emission line of hydro...
Infrared absorption lines of H+3, including the metastable R(3,3)l line, have been observed toward e...
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in ...
We have carried out a sensitive high-latitude (|b| > 15?) HI 21 cm-line absorption survey towards 10...
We present a 21-cm emission-absorption study towards extragalactic sources in the Canadian Galactic ...
Author Institution: Subaru Telescope, 650, North A'ohoku Place, Hilo HI 96720/Institute for Astronom...
We present a follow-up observation on Geballe and Oka (2010, ApJ, 709, L70), who found high column d...
A gaussian analysis of the HI absorption spectrum of Sgr A obtained with the Parkes Interferometer h...
Context. In the near- to mid-infrared wavelength domain, bright continuum sources in the central par...
The OH distribution in the Sgr A Complex has been observed in the 1612-, 1665-, 1667- and 1720-MHz O...
We present a follow-up observation on Geballe and Oka (2010, ApJ, 709, L70), who found high column d...
Author Institution: Department of Astronomy and Astrophysics and Department of Chemistry, University...
Restricted Access.We present the highest resolution Very Large Array 74 MHz images of a ~ 10 degree ...
We present high-resolution (R = 20000) spectroscopy of H+3 absorption toward the luminous Galactic c...
We present an H I absorption survey of the central 250 pc of the Galaxy. Very Large Array observatio...
The neutral atomic gas content of galaxies is usually studied in the HI 21 cm emission line of hydro...
Infrared absorption lines of H+3, including the metastable R(3,3)l line, have been observed toward e...
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in ...
We have carried out a sensitive high-latitude (|b| > 15?) HI 21 cm-line absorption survey towards 10...
We present a 21-cm emission-absorption study towards extragalactic sources in the Canadian Galactic ...
Author Institution: Subaru Telescope, 650, North A'ohoku Place, Hilo HI 96720/Institute for Astronom...
We present a follow-up observation on Geballe and Oka (2010, ApJ, 709, L70), who found high column d...
A gaussian analysis of the HI absorption spectrum of Sgr A obtained with the Parkes Interferometer h...
Context. In the near- to mid-infrared wavelength domain, bright continuum sources in the central par...
The OH distribution in the Sgr A Complex has been observed in the 1612-, 1665-, 1667- and 1720-MHz O...
We present a follow-up observation on Geballe and Oka (2010, ApJ, 709, L70), who found high column d...
Author Institution: Department of Astronomy and Astrophysics and Department of Chemistry, University...
Restricted Access.We present the highest resolution Very Large Array 74 MHz images of a ~ 10 degree ...
We present high-resolution (R = 20000) spectroscopy of H+3 absorption toward the luminous Galactic c...