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A new catalog of 8382 close quasar-galaxy pairs is presented. The catalog was composed using published catalogs of quasars and active galactic nuclei containing 11358 objects, as well as the LEDA catalog of galaxies, which contains on the…

天体物理学 · 物理学 2009-11-07 Yu. L. Bukhmastova

Observations at various wavelengths of late B-type stars exhibiting strong overabundances of the chemical elements Hg and Mn in their atmospheres indicate that these stars are frequently found in binary and multiple systems. We intend to…

太阳与恒星天体物理 · 物理学 2015-05-20 M. Schöller , S. Correia , S. Hubrig , N. Ageorges

We carried out a systematic search for new star clusters in a field of 5$^{\circ} \times5^{\circ}$ centred close to the Galactic Nucleus using the infrared JHK$_s$ 2MASS Survey archive. In addition we searched for embedded clusters in the…

天体物理学 · 物理学 2007-05-23 C. M. Dutra , E. Bica

Filaments of galaxies are known to stretch between galaxy clusters at all redshifts in a complex manner. In this Letter, we present an analysis of the frequency and distribution of inter-cluster galaxy filaments selected from the 2dF Galaxy…

天体物理学 · 物理学 2009-11-10 Kevin A. Pimbblet , Michael J. Drinkwater , Mary C. Hawkrigg

Aims. We aim to identify and classify BCs using high-precision astrometric and kinematic data, and to investigate their physical properties, mutual gravitational interactions, and formation rates. Methods. We used a comprehensive star…

星系天体物理 · 物理学 2025-10-08 Guimei Liu , Yu Zhang , Jing Zhong , Songmei Qin , Yueyue Jiang , Li Chen

Over the last decades, numerous wide (>1000 AU) binaries have been discovered in the Galactic field and halo. The origin of these wide binaries cannot be explained by star formation or by dynamical interactions in the Galactic field. We…

星系天体物理 · 物理学 2009-09-08 M. B. N. Kouwenhoven , S. P. Goodwin , Richard J. Parker , M. B. Davies , D. Malmberg , P. Kroupa

The distribution of smaller satellite galaxies around large central galaxies has attracted attention because peculiar spatial and kinematic configurations have been detected in some systems. A particularly striking example of such behavior…

星系天体物理 · 物理学 2016-10-26 Noam I Libeskind , Quan Guo , Elmo Tempel , Rodrigo Ibata

The fraction of binary stars is an important ingredient to interpret globular cluster dynamical evolution and their stellar population. We investigate the properties of main-sequence binaries measured in a uniform photometric sample of 59…

With the release of Gaia data, the number of known Galactic open clusters (OCs) has increased rapidly, providing an excellent opportunity to confirm more binary open clusters in the Milky Way. Using a recently released OC catalogue, we…

星系天体物理 · 物理学 2025-08-28 Zhongmu Li , Zhanpeng Zhu

We present a catalog of Galactic star clusters, associations and candidates with 10978 entries. This multi-band catalog was constructed over 20 years, starting with visual inspections on the Digital Sky Survey and incremented with the…

星系天体物理 · 物理学 2019-01-02 Eduardo Bica , Daniela B. Pavani , Charles J. Bonatto , Eliade F. Lima

We report on a high-spatial-resolution survey for binary stars in the periphery of the Orion Nebula Cluster, at 5 - 15 arcmin (0.65 - 2 pc) from the cluster center. We observed 228 stars with adaptive optics systems, in order to find…

A simulated binary star catalogue is created that represents the full sky distribution of stars, excluding those with galactic latitude $|b|<10\degr$, down to $m_v < 15$. The catalogue is compatible with observed magnitude and number…

天体物理学 · 物理学 2009-11-07 Pasi Nurmi , Henri M. J. Boffin

Most Sun-like and higher-mass stars reside in systems that include one or more gravitationally bound stellar companions. These systems offer an important probe of planet formation in the most common stellar systems, while also providing key…

地球与行星天体物理 · 物理学 2025-03-12 Joseph E. Hand , Malena Rice , Konstantin Gerbig

We have observed the recently discovered rich star cluster GLIMPSE-C01 for 46 ks with the Chandra X-ray Observatory. Seventeen X-ray sources with luminosities greater than 0.6e31 ergs/s were discovered, one of which is likely a quiescent…

天体物理学 · 物理学 2007-08-27 D. Pooley , S. Rappaport , A. Levine , E. Pfahl , J. Schwab

Luminous elliptical galaxies generally display a rich star cluster system, whose properties provide strong constraints on the physics of galaxy formation and evolution. Star cluster system studies, however, concentrate on galaxies located…

天体物理学 · 物理学 2009-11-13 B. X. Santiago

We present a new, objectively defined catalog of candidate galaxy clusters based on the galaxy catalogs from the Digitized Second Palomar Observatory Sky Survey (DPOSS). This cluster catalog, derived from the best calibrated plates in the…

The crossing of the Galactic disk by a Globular Cluster could produce star formation due to gravitational focussing or compression of disk material. We report on simulations of the effect on disk material which reveal that the crossing can…

天体物理学 · 物理学 2008-11-20 D. Vande Putte , Mark Cropper

Binary interactions are commonplace among massive stars, giving rise observed phenomena such as X-ray binaries, stripped stars & supernovae, and gravitational-wave sources. The multiplicity properties of massive stars thus represent a…

太阳与恒星天体物理 · 物理学 2024-10-22 Tomer Shenar

We applied the newly developed rose diagram overlay method to detect the layered structure of 88 nearby open clusters ($\leq$500~pc) on the three projections after the distance correction of their member stars, based on the catalog in…

星系天体物理 · 物理学 2023-05-18 Qingshun Hu , Yu Zhang , Ali Esamdin , Hong Wang , Mingfeng Qin

We have developed a star-counting algorithm and tested it on the 2MASS star catalog to search for density enhancements significantly above the field in Galactic latitude $|b|<50^{\circ}$. Nearly 500 open clusters are "rediscovered", along…

太阳与恒星天体物理 · 物理学 2012-02-21 C. C. Lin , W. P. Chen , E. A. Magnier