International audienceAbstract In this work, we demonstrate that the Perseus Arm is not a continuous structure of molecular gas in the second quadrant. We first show that the observed, distanced-resolved velocity structure of the Galaxy in the outer disk is capable of creating illusory spiral arms, as was first proposed by Burton. Second, we measure the distances to a collection of CO clouds at velocities consistent with the Perseus arm with 135° < l < 160°. We find these distances using 3D dust maps from Green et al. We determine that these molecular clouds do not preferentially lie at the distance of a purported Perseus arm but rather extend over 3 kpc in distance, with some evidence for a closer, high pitch angle structure between 1 and ...
We present a map of the spiral structure of the Galaxy, as traced by molecular carbon monosulphide (...
Context. The spiral structure of the Milky Way is not yet well determined. The keys to und...
Whereas it is well established that spiral arms are important agents driving the evolution of the ga...
International audienceAbstract In this work, we demonstrate that the Perseus Arm is not a continuous...
This is the final version. Available from Royal Astronomical Society / Oxford University Press via t...
We have measured the distance to the massive star-forming region W3OH in the Perseus spiral arm of t...
We have measured the distance to the massive star-forming region W3OH in the Perseus Spiral arm of t...
We present results of a survey of 14 star-forming regions from the Perseus spiral armin CS (2–1) and...
It was in 1864 that the first clues as to the nature of the space between stars were first identifie...
Here we propose a two step approach to provide new insights on the outer spiral arm pattern of the M...
We present high-resolution smoothed particle hydrodynamics simulations of a region of gas flowing in...
We report the detection in CO of the far-side counterpart of the well-known expanding 3-Kpc Arm in t...
Making use of a new high-resolution spiral galaxy simulation as well as Gaia DR2 and EDR3 data compl...
Many features near the Galactic Center have been called \u20183-kiloparsec arms\u2019. We reached a ...
Kinematic distances to 750 molecular clouds identified in the [superscript 13]CO J = 1 → 0 Boston Un...
We present a map of the spiral structure of the Galaxy, as traced by molecular carbon monosulphide (...
Context. The spiral structure of the Milky Way is not yet well determined. The keys to und...
Whereas it is well established that spiral arms are important agents driving the evolution of the ga...
International audienceAbstract In this work, we demonstrate that the Perseus Arm is not a continuous...
This is the final version. Available from Royal Astronomical Society / Oxford University Press via t...
We have measured the distance to the massive star-forming region W3OH in the Perseus spiral arm of t...
We have measured the distance to the massive star-forming region W3OH in the Perseus Spiral arm of t...
We present results of a survey of 14 star-forming regions from the Perseus spiral armin CS (2–1) and...
It was in 1864 that the first clues as to the nature of the space between stars were first identifie...
Here we propose a two step approach to provide new insights on the outer spiral arm pattern of the M...
We present high-resolution smoothed particle hydrodynamics simulations of a region of gas flowing in...
We report the detection in CO of the far-side counterpart of the well-known expanding 3-Kpc Arm in t...
Making use of a new high-resolution spiral galaxy simulation as well as Gaia DR2 and EDR3 data compl...
Many features near the Galactic Center have been called \u20183-kiloparsec arms\u2019. We reached a ...
Kinematic distances to 750 molecular clouds identified in the [superscript 13]CO J = 1 → 0 Boston Un...
We present a map of the spiral structure of the Galaxy, as traced by molecular carbon monosulphide (...
Context. The spiral structure of the Milky Way is not yet well determined. The keys to und...
Whereas it is well established that spiral arms are important agents driving the evolution of the ga...