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Open AccessJournal ArticleDOI

The spatial distribution of star formation in the solar neighbourhood: do all stars form in dense clusters?

TLDR
In this article, a global study of low mass, young stellar object (YSO) surface densities in nearby star forming regions based on a comprehensive collection of Spitzer Space Telescope surveys is presented.
Abstract
We present a global study of low mass, young stellar object (YSO) surface densities (�) in nearby (< 500 pc) star forming regions based on a comprehensive collection of Spitzer Space Telescope surveys. We show that the distribution of YSO surface densities in the solar neighbourhood is a smooth distribution, being adequately described by a lognormal function from a few to 10 3 YSOs per pc 2 , with a peak at � 22 stars pc

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Journal ArticleDOI

Star Formation in the Milky Way and Nearby Galaxies

TL;DR: In this paper, the authors review progress over the past decade in observations of large-scale star formation, with a focus on the interface between extragalactic and Galactic studies.
Journal ArticleDOI

Stellar Multiplicity

TL;DR: In this article, the authors summarize the current empirical knowledge of stellar multiplicity for Main Sequence stars and brown dwarfs, as well as among populations of Pre-Main Sequence stars, and embedded protostars.
Journal ArticleDOI

On the fraction of star formation occurring in bound stellar clusters

TL;DR: In this article, the authors present a theoretical framework in which bound stellar clusters arise naturally at the high-density end of the hierarchy of the interstellar medium (ISM) and due to short free-fall times, these high density regions achieve high local star formation efficiencies, enabling them to form bound clusters.
Journal ArticleDOI

The big problems in star formation: The star formation rate, stellar clustering, and the initial mass function

TL;DR: A review of the current state of the field of star formation can be found in this article, focusing on three central questions: What controls the rate at which gas in a galaxy converts to stars? What determines how those stars are clustered, and what fraction of the stellar population ends up in gravitationally-bound structures?
References
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Journal ArticleDOI

Embedded Clusters in Molecular Clouds

TL;DR: The first extensive catalog of galactic embedded clusters is compiled, finding that the embedded cluster birthrate exceeds that of visible open clusters by an order of magnitude or more indicating a high infant mortality rate for protocluster systems.
Journal ArticleDOI

Disk Frequencies and Lifetimes in Young Clusters

TL;DR: In this paper, the authors report the results of the first sensitive L-band survey of the intermediate-age (2.5-30 Myr) clusters NGC 2264, NGC 2362, and NGC 1960.
Book

Protostars and Planets V

TL;DR: Protostars and Planets V as mentioned in this paper provides a detailed and up-to-date picture of star and planet formation, including the formation and early evolution of our own solar system.
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