G86.5+59.6 is a degree-sized high latitude cloud originally selected for investigation by Heiles, Reach, and Koo (1988) on the basis of its appearance on the IRAS Skyflux images at 60 and 100 micrometers. Because of the interesting possibility that this is an intermediate velocity cloud colliding with HI in the Galactic plane, we have examined this region further, both at low resolution over an extended field to provide some context and at higher (arcminute) resolution within the cloud
Photometric and spectroscopic observations have been made of northern hemisphere early type stars at...
We have mapped 1 deg 2 region toward a high latitude H ii region S73 (l; b) = (37 ffi :69; 44 f...
We present a high-resolution study of five high-velocity clouds in the Magellanic Leading Arm region...
An atlas of the Galactic plane (-4.°7 < b < 4.°7), along with the molecular clouds in Orion, ? Oph, ...
We have measured the velocity and equivalent widths of the optical interstellar lines in a group of ...
The Infrared Astronomy Satellite (IRAS) Galactic Plane Surface Brightness Images were used to identi...
We present high-resolution (R = 400 000) observations of interstellar Ca II and Na I absorption line...
We have created a map of the large-scale infrared surface brightness in excess of that associated wi...
A CO survey of 342 Infrared Excess Clouds (IRECs) distributed uniformly across the sky is presented....
The high latitude dark cloud L1642 in the 21 cm H I region was mapped using a 100 m radio telescope....
We present distance estimates to a set of high-latitude intermediate-velocity HI clouds. We explore ...
Context. Intermediate-velocity clouds (IVCs) are HI halo clouds that are likely related to a Galacti...
The goal of this project was to develop new tools for the analysis of the structure of densely sampl...
We present near-infrared (JHKL) photometry of 103 southern stars located behind translucent interste...
Because infrared emission is a very good tracer of mass at high latitudes, by combining it with HI o...
Photometric and spectroscopic observations have been made of northern hemisphere early type stars at...
We have mapped 1 deg 2 region toward a high latitude H ii region S73 (l; b) = (37 ffi :69; 44 f...
We present a high-resolution study of five high-velocity clouds in the Magellanic Leading Arm region...
An atlas of the Galactic plane (-4.°7 < b < 4.°7), along with the molecular clouds in Orion, ? Oph, ...
We have measured the velocity and equivalent widths of the optical interstellar lines in a group of ...
The Infrared Astronomy Satellite (IRAS) Galactic Plane Surface Brightness Images were used to identi...
We present high-resolution (R = 400 000) observations of interstellar Ca II and Na I absorption line...
We have created a map of the large-scale infrared surface brightness in excess of that associated wi...
A CO survey of 342 Infrared Excess Clouds (IRECs) distributed uniformly across the sky is presented....
The high latitude dark cloud L1642 in the 21 cm H I region was mapped using a 100 m radio telescope....
We present distance estimates to a set of high-latitude intermediate-velocity HI clouds. We explore ...
Context. Intermediate-velocity clouds (IVCs) are HI halo clouds that are likely related to a Galacti...
The goal of this project was to develop new tools for the analysis of the structure of densely sampl...
We present near-infrared (JHKL) photometry of 103 southern stars located behind translucent interste...
Because infrared emission is a very good tracer of mass at high latitudes, by combining it with HI o...
Photometric and spectroscopic observations have been made of northern hemisphere early type stars at...
We have mapped 1 deg 2 region toward a high latitude H ii region S73 (l; b) = (37 ffi :69; 44 f...
We present a high-resolution study of five high-velocity clouds in the Magellanic Leading Arm region...