We present an expanded distance catalog for 1710 molecular cloud structures identified in the Bolocam Galactic Plane Survey (BGPS) version 2, representing a nearly threefold increase over the previous BGPS distance catalog. We additionally present a new method for incorporating extant data sets into our Bayesian distance probability density function (DPDF) methodology. To augment the dense-gas tracers (e.g., HCO+ (3-2), NH3(1,1)) used to derive line-of-sight velocities for kinematic distances, we utilize the Galactic Ring Survey (GRS) (CO)-C-13(1-0) data to morphologically extract velocities for BGPS sources. The outline of a BGPS source is used to select a region of the GRS (CO)-C-13 data, along with a reference region to subtract envelopi...
We present the results of a Green Bank Telescope survey of NH3(1,1), (2,2), (3,3) lines toward 631 B...
We present distances to 76 medium-sized molecular clouds and an extra large-scale molecular cloud in...
We present a new technique to determine distances to major star-forming regions across the Perseus M...
We present an expanded distance catalog for 1710 molecular cloud structures identified in the Boloca...
We present an expanded distance catalog for 1,710 molecular cloud structures identified in the Boloc...
We use the distance probability density function formalism of Ellsworth-Bowers et al. to derive phys...
Kinematic distances to 750 molecular clouds identified in the [superscript 13]CO J = 1 → 0 Boston Un...
We present a new distance estimation method for dust-continuum-identified molecular cloud clumps. Re...
The Milky Way Galaxy serves as a vast laboratory for studying the dynamics and evolution of the dens...
The H2O Southern Galactic Plane Survey (HOPS) has mapped a 100° strip of the Galactic plane (-70° > ...
Context. New-generation spectroscopic surveys of the Milky Way plane have been revealing the structu...
We present the results of a Green Bank Telescope survey of NH(3)(1,1), (2,2), (3,3) lines toward 631...
International audienceThe H2O Southern Galactic Plane Survey (HOPS) has mapped a 100° strip of the G...
We present a new catalog of spectrophotometric distances and line of sight systemic velocities to 10...
The H₂O Southern Galactic Plane Survey (HOPS) has mapped a 100 degrees strip of the Galactic plane (...
We present the results of a Green Bank Telescope survey of NH3(1,1), (2,2), (3,3) lines toward 631 B...
We present distances to 76 medium-sized molecular clouds and an extra large-scale molecular cloud in...
We present a new technique to determine distances to major star-forming regions across the Perseus M...
We present an expanded distance catalog for 1710 molecular cloud structures identified in the Boloca...
We present an expanded distance catalog for 1,710 molecular cloud structures identified in the Boloc...
We use the distance probability density function formalism of Ellsworth-Bowers et al. to derive phys...
Kinematic distances to 750 molecular clouds identified in the [superscript 13]CO J = 1 → 0 Boston Un...
We present a new distance estimation method for dust-continuum-identified molecular cloud clumps. Re...
The Milky Way Galaxy serves as a vast laboratory for studying the dynamics and evolution of the dens...
The H2O Southern Galactic Plane Survey (HOPS) has mapped a 100° strip of the Galactic plane (-70° > ...
Context. New-generation spectroscopic surveys of the Milky Way plane have been revealing the structu...
We present the results of a Green Bank Telescope survey of NH(3)(1,1), (2,2), (3,3) lines toward 631...
International audienceThe H2O Southern Galactic Plane Survey (HOPS) has mapped a 100° strip of the G...
We present a new catalog of spectrophotometric distances and line of sight systemic velocities to 10...
The H₂O Southern Galactic Plane Survey (HOPS) has mapped a 100 degrees strip of the Galactic plane (...
We present the results of a Green Bank Telescope survey of NH3(1,1), (2,2), (3,3) lines toward 631 B...
We present distances to 76 medium-sized molecular clouds and an extra large-scale molecular cloud in...
We present a new technique to determine distances to major star-forming regions across the Perseus M...