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[1509.01082] Understanding star formation in molecular clouds III ...


[1509.01082] Understanding star formation in molecular clouds III ...

Star-forming clouds can best be characterized by lognormal PDFs for the lower N range and a power-law tail for higher N, commonly attributed to ...

Understanding star formation in molecular clouds. III. Probability ...

We report here on PDFs that were obtained from observations of 12CO, 13CO, C18O, CS, and N2H+ in the Cygnus X North region, and make a comparison to a PDF that ...

Understanding star formation in molecular clouds III. Probability ...

Star-forming clouds can best be characterized by lognormal PDFs for the lower N range and a power-law tail for higher N, commonly attributed to ...

arXiv:1509.01082v2 [astro-ph.GA] 15 Jan 2016

Understanding star formation in molecular clouds. III. Probability distribution functions of molecular lines in Cygnus X. N.Schneider1,2, S ...

Understanding star formation in molecular clouds III. Probability ...

Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X · N.Schneider, S.

How much of a molecular cloud can end up as "starstuff"?

This quantity is referred to as star formation efficiency (SFE) by astronomers who study star formation and galaxy evolution.

Star Formation in Molecular Clouds - Mark R. Krumholz

Abstract: Star formation is one of the least understood processes in cosmic evolution. It is difficult to formulate a general theory for star formation in part ...

The Densities and Dynamics of Molecular Clouds in Spiral Galaxies

“Understanding star formation in molecular clouds. ... arXiv: 1509.01082. Schneider, S. and B. G. ... “On the nature of star-forming filaments - II.

Publications: Zentrum für Astronomie

... Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X, eprint arXiv: 1509.01082 (2015).

Understanding Star Formation in the Perseus Molecular Cloud

For typical molcular cloud conditions (i.e., n ≈ 102 cm−3 and temperature T ≈ 10 K), the Jeans mass is ~500 M . Molecular clouds contain tens of thousands of ...

How do stars form inside molecular clouds? What is the difference ...

That is where most stars are formed. Certain galaxies are full of these clouds, usually formed from the explosion of previous blue giant stars ...

Star Formation in Molecular Clouds

However, at the high densities where stars form, hydrogen tends to be molecular rather than atomic, and H2 is extremely hard to observe directly. To understand ...

Understanding star formation in molecular clouds - R Discovery

We present N-PDFs of 29 Galactic regions obtained from Herschel imaging at high angular resolution (18″), covering diffuse and quiescent clouds, ...

New Astronomy Finding Uncovers the Mystery of Star Formation at ...

The discovered 23 molecular clouds appear different from their counterparts in typical star-forming sites in galaxies. The large bodies of these ...