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相关论文: Large-scale expansion of OB stars in Cygnus

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OB associations play an important role in Galactic evolution, though their origins and dynamics remain poorly studied, with only a small number of systems analysed in detail. In this paper we revisit the existence and membership of the…

太阳与恒星天体物理 · 物理学 2024-11-20 Alexis L. Quintana , Nicholas J. Wright

We present 3-dimensional kinematical observations of the massive OB association Cygnus OB2 to identify the mechanisms responsible for disrupting young star clusters. The picture revealed by these observations is of a highly-substructured,…

太阳与恒星天体物理 · 物理学 2012-08-02 Nicholas J. Wright , Herve Bouy , Jeremy J. Drake , Janet E. Drew , Mario Guarcello , David Barrado y Navacues

OB associations are the prime star forming sites in galaxies. However the detailed formation process of such stellar systems still remains a mystery. In this context, identifying the presence of substructures may help tracing the footprints…

太阳与恒星天体物理 · 物理学 2020-12-09 Beomdu Lim , Yael Naze , Eric Gosset , Gregor Rauw

We examine substructure and mass segregation in the massive OB association Cygnus OB2 to better understand its initial conditions. Using a well understood Chandra X-ray selected sample of young stars we find that Cyg OB2 exhibits…

太阳与恒星天体物理 · 物理学 2015-06-17 Nicholas J. Wright , Richard J. Parker , Simon P. Goodwin , Jeremy J. Drake

OB associations are the prevailing star forming sites in the Galaxy. Up to now, the process of how OB associations were formed remained a mystery. A possible process is self-regulating star formation driven by feedback from massive stars.…

Cygnus OB2 provides a unique insight into the high-mass stellar content in one of the largest groups of young massive stars in our Galaxy. Although several studies of its massive population have been carried out over the last decades, an…

太阳与恒星天体物理 · 物理学 2020-10-21 S. R. Berlanas , A. Herrero , F. Comerón , S. Simón-Díaz , D. J. Lennon , A. Pasquali , J. Maíz Apellániz , A. Sota , A. Pellerín

The compact association Cygnus OB2 is known to contain a large population of massive stars, but its total mass is currently a matter of debate. While recent surveys have uncovered large numbers of OB stars in the area around Cyg OB2,…

天体物理学 · 物理学 2015-05-13 Ignacio Negueruela , Amparo Marco , Artemio Herrero , Simon Clark

We investigate the formation of star clusters in an unbound GMC, where the supporting kinetic energy is twice as large as the cloud's self-gravity. This cloud manages to form a series of star clusters and disperse, all within roughly 2…

天体物理学 · 物理学 2014-10-13 Paul C. Clark , Ian A. Bonnell , Hans Zinnecker , Matthew R. Bate

We have compiled a significantly updated and comprehensive census of massive stars in the nearby Cygnus OB2 association by gathering and homogenising data from across the literature. The census contains 169 primary OB stars, including 52…

太阳与恒星天体物理 · 物理学 2015-06-23 Nicholas J. Wright , Janet E. Drew , Michael Mohr-Smith

The formation of stars in massive clusters is one of the main modes of the star formation process. However, the study of massive star forming regions is hampered by their typically large distances to the Sun. One exception to this is the…

Kinematic studies of young stars and star clusters have increased our understanding of the process of star formation and evolution in the Milky Way. FU Orionis objects are a specific class of young stellar object notable for their extremely…

星系天体物理 · 物理学 2025-10-01 Tamojeet Roychowdhury , Lynne A. Hillenbrand

Cygnus OB2 is the nearest example of a massive star forming region, containing over 50 O-type stars and hundreds of B-type stars. We have analyzed two Chandra pointings in Cyg OB2, detecting ~1700 X-ray sources, of which ~1450 are thought…

太阳与恒星天体物理 · 物理学 2015-05-27 Nicholas J. Wright , Jeremy J. Drake , Janet E. Drew , Jorick S. Vink

We perform a large-scale hydrodynamic simulation of a massive star cluster whose stellar population mimics that of the Cygnus OB2 association. The main-sequence stars are first simulated during 1.6 Myr, until a quasi-stationary state is…

Cygnus OB2 is the nearest example of a massive star forming region, containing over 50 O-type stars and hundreds of B-type stars. We have analysed the properties of young stars in two fields in Cyg OB2 using the recently published deep…

太阳与恒星天体物理 · 物理学 2015-05-18 Nicholas J. Wright , Jeremy J. Drake , Janet E. Drew , Jorick S. Vink

Radiative feedback from massive stars can potentially trigger star formation in the surrounding molecular gas. Inspired by the case of radiatively driven implosion in M16 or Eagle Nebula, we analyze a similar case of star formation observed…

太阳与恒星天体物理 · 物理学 2018-09-12 Soumen Deb , Roland Kothes , Erik Rosolowsky

We investigate the possible existence of an extended halo of early-type stars around Cygnus OB2, which is hinted at by near-infrared color-color diagrams, and its relationship to Cygnus OB2 itself, as well as to the nearby association…

天体物理学 · 物理学 2009-11-13 F. Comeron , A. Pasquali , F. Figueras , J. Torra

We discuss observational evidence for sequential and triggered star formation in OB associations. We first review the star formation process in the Scorpius-Centaurus OB association, the nearest OB association to the Sun, where several…

天体物理学 · 物理学 2009-11-11 Thomas Preibisch , Hans Zinnecker

We present an observational study of small-scale feedback processes operating in the star-forming region located in the wall of the expanding supershell around the Cyg OB1 association. The interstellar gas and dust content and pre-stellar…

The main objective of this study is the characterization of the velocity field in the Cygnus OB1 association using the radial velocity data currently available in the literature. This association is part of a larger star-forming complex…

星系天体物理 · 物理学 2017-01-11 M. T. Costado , E. J. Alfaro , M. Gonzalez , L. Sampedro

In our Galaxy, star formation occurs in a variety of environments, with a large fraction of stars formed in clusters hosting massive stars. OB stars have an important feedback on the evolution of protoplanetary disks around nearby young…

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