Star|forming regions of the Aquila rift cloud complex

Star-forming regions of the Aquila rift cloud complex

In the present part of our survey we search for ammonia emitters in the Aquila rift complex, which trace the densest regions of molecular clouds.

Star-forming regions of the Aquila rift cloud complex - I. NH3 tracers ...

Most stars are formed in high-density environments (n > 104 cm-3) and emit lines of diverse molecular transitions. In the present part of our survey we search ...

Star-forming regions of the Aquila rift cloud complex. I. NH 3 tracers ...

Most stars are formed in high-density environments (n > 104 cm-3) and emit lines of diverse molecular transitions. In the present part of our survey we search ...

Star-forming regions of the Aquila rift cloud complex. II. Turbulence ...

Abstract page for arXiv paper 1405.7492: Star-forming regions of the Aquila rift cloud complex. II. Turbulence in molecular cores probed by ...

Star-forming regions of the Aquila rift cloud complex. I. NH3 tracers ...

Abstract:(Abridged) Aims. In the present part of our survey we search for ammonia emitters in the Aquila rift complex which trace the ...

Star-forming regions of the Aquila rift cloud complex-I. NH_{3 ...}

... Aquila rift complex, which trace the densest regions of molecular clouds. Methods. From a CO survey carried out with the Delingha 14-m telescope we selected ...

The Aquila Rift star-forming complex viewed by Herschel and Planck

The Aquila Rift is a region that spans the constellations of Aquila and Serpens and contains the Aquila Rift cloud complex. This harbours ...

Star-forming regions of the Aquila rift cloud complex. II. Turbulence ...

NASA/ADS · Star-forming regions of the Aquila rift cloud complex. II. Turbulence in molecular cores probed by NH3 emission.

(PDF) Star-forming regions of the Aquila rift cloud complex. I. NH3 ...

Star-forming regions of the Aquila rift cloud complex. I. NH3 tracers of dense molecular cores. March 2013; Astronomy and Astrophysics 553. 553. DOI:10.1051 ...

Serpens–Aquila Rift - Wikipedia

Therefore, the clouds in the Serpens-Aquila Rift block light from background stars in the disk of the Galaxy, forming the dark rift. The complex is located in a ...

Star Formation in the Aquila Rift

They coincide with regions of relatively lower extinction, which suggests that they are on the far side of the W40 cloud complex but still related to W40.

Star-forming regions of the Aquila rift cloud complex - OUCI

Star-forming regions of the Aquila rift cloud complex · List of references · Publications that cite this publication.

Small Molecular Clouds Possibly Associated with the Aquila Rift

this complex, < 0.03%, by taking the mass of the can- didate to be 1 M®. This is much lower than those in typical low-mass star-forming regions, for example Tau ...

A Detailed Analysis of the Cloud Structure and Dynamics in Aquila Rift

We have studied the active star-forming regions W40 and Serpens South in the Aquila Rift complex. We observed a region of 1 square degree around W40 and ...

Star-forming regions of the Aquila rift cloud complex - OUCI

Star-forming regions of the Aquila rift cloud complex ... Authors: S. A. Levshakov; C. Henkel; D. Reimers; M. Wang; R. Mao; H. Wang; Y.

Star Formation in ... - OFFICIAL Denver Museum of Nature & Science

... star formation in the W40 cluster and the Aquila Rift region. ... star-forming regions ... cloud complex but still related to W40. Excess Star Count Based on 30NN.

Where are all the Young Stars in Aquila? - Bernhard Hubl

Aquila molecular cloud complex, however, few young stars are known to be located in the area, and only one is directly associated with the Rift. In contrast ...

Star-forming regions of the Aquila rift cloud complex. I. NH3 tracers ...

(Abridged) Aims. In the present part of our survey we search for ammonia emitters in the Aquila rift complex which trace the densest regions ...

Small Molecular Clouds Possibly Associated with the Aquila Rift ...

A cloud complex consisting of 64 small clouds has been discovered in −25° ≲ b ≲ −12°; at a distance of 220 pc, its height from the galactic plane is ∼ 50–100 pc ...

Ammonia observations towards the Aquila Rift cloud complex

We surveyed the Aquila Rift complex including the Serpens South and W40 region in the NH$_3$(1,1) and (2,2) transitions making use of the ...