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相关论文: Testing the two planes of satellites in the Centau…

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We study the resolved stellar populations of dwarf galaxies in the nearby Centaurus A/M83 group of galaxies. Our goal is to characterize their evolutionary history and to investigate eventual similarities or differences with the dwarf…

宇宙学与河外天体物理 · 物理学 2015-05-27 D. Crnojević , E. K. Grebel , A. A. Cole

The existence and prevalence of planar, co-rotating distributions of satellite galaxies around L* host galaxies in the local universe remains a subject of ongoing debate. Despite numerous observational efforts over the past decade, a…

星系天体物理 · 物理学 2026-02-25 Ethan Crosby , Marcel S. Pawlowski , Oliver Müller , Helmut Jerjen

We have carried out surface photometry of four bright known members and a number of new possible LSB companions of the IC 65 (LGG 16) group of galaxies. The purpose of the present study is twofold: (a) a search for new LSB dwarf members and…

天体物理学 · 物理学 2007-05-23 J. Vennik , U. Hopp

Both major galaxies in the Local Group (LG) are surrounded by thin planes of mostly co-orbiting satellite galaxies, the vast polar structure (VPOS) around the Milky Way (MW) and the Great Plane of Andromeda (GPoA) around M31. We summarize…

宇宙学与河外天体物理 · 物理学 2015-06-16 Marcel S. Pawlowski , Pavel Kroupa , Helmut Jerjen

We examine the prevalence, longevity, and causes of planes of satellite dwarf galaxies, as observed in the Local Group. We use 14 Milky Way/Andromeda-(MW/M31) mass host galaxies from the FIRE-2 simulations. We select the 14 most massive…

The galaxy system around NGC4490 was recently highlighted to display a flattened, kinematically correlated structure reminiscent of satellite galaxy planes around other hosts. Since known satellite planes are in tension with $\Lambda$CDM…

Current models of galaxy formation predict that galaxy pairs of comparable magnitudes should become increasingly rare with decreasing luminosity. This seems at odds with the relatively high frequency of pairings among dwarf galaxies in the…

宇宙学与河外天体物理 · 物理学 2015-06-12 Azadeh Fattahi , Julio F. Navarro , Else Starkenburg , Christopher R. Barber , Alan W. McConnachie

We present the survey strategy and early results of the "Satellites Around Galactic Analogs" (SAGA) Survey. The SAGA Survey's goal is to measure the distribution of satellite galaxies around 100 systems analogous to the Milky Way down to…

Context: The nearby pair of solar-type stars Alpha Centauri is a favorable target for an imaging search for extrasolar planets. Indications exist that the gravitational mass of Alpha Cen B could be higher than its modeled mass, the…

天体物理学 · 物理学 2016-08-15 Pierre Kervella , Frédéric Thévenin

We present a detailed characterization of planes of satellite galaxies in the Milky Way (MW) and M31. For a positional analysis, we introduce an extension to the `4-galaxy-normal density plot' method \citep[][P13]{Pawlowski13}. It finds the…

星系天体物理 · 物理学 2020-11-11 Isabel Santos-Santos , Rosa Dominguez-Tenreiro , Marcel S. Pawlowski

In the last years, a new generation of large-scale imaging surveys have probed wide field regions around some nearby galaxies at unprecedented low surface brightness regime (~28.0-29.0 mag arcsec^-2). This offers a chance of discovering…

Multiple structures within stellar groups are an intriguing subject for theoretical and observational studies of stellar formation. With the accuracy and completeness of data from Gaia Data Release 3, we now have new opportunities to detect…

星系天体物理 · 物理学 2025-10-14 Mohammad Noormohammadi , Atefeh Javadi , Mehdi Khakian Ghomi

Some galaxies such as the Milky Way and Andromeda display coherently rotating satellite planes, posing tensions with cosmological simulations. NGC 2750 has emerged as an additional candidate system hosting a co-rotating group of galaxies.…

We report on the HI content of an isolated, compact group of 6 dwarf galaxies at a distance of 145 Mpc. The distribution and kinematics of the HI, including multiple gaseous bridges, indicate the group is a gravitationally bound system. The…

We analyse the properties of three unusual dwarf galaxies in the Centaurus A group discovered with the HIPASS survey. From their optical morphology they appear to be low surface brightness dwarf spheroidals, yet they are gas-rich…

天体物理学 · 物理学 2008-11-26 M. Grossi , M. J. Disney , B. J . Pritzl , P. M. Knezek , J. S. Gallagher , R. F. Minchin , K. C. Freeman

We present results of two 21-cm HI surveys performed with the Australia Telescope Compact Array in the nearby Centaurus A and Sculptor galaxy groups. These surveys are sensitive to compact HI clouds and galaxies with HI masses as low as…

天体物理学 · 物理学 2009-11-07 W. J. G. de Blok , M. A. Zwaan , M. Dijkstra , F. H. Briggs , K. C. Freeman

We report the discovery of a large population of dwarf irregular galaxies in the two nearest groups of galaxies outside the Local Group, the Sculptor and the Centaurus A groups (2.5 and 3.5 Mpc). Total areas of approximately 940 and 910…

天体物理学 · 物理学 2009-12-10 Stephanie Cote , Ken Freeman , Claude Carignan , Peter Quinn

We use more than a decade of radial velocity measurements for $\alpha$ Cen A, B, and Proxima Centauri from HARPS, CHIRON, and UVES to identify the $M \sin i$ and orbital periods of planets that could have been detected if they existed. At…

地球与行星天体物理 · 物理学 2017-12-27 Lily L. Zhao , Debra A. Fischer , John M. Brewer , Matt Giguere , Bárbara Rojas-Ayala

We report detailed studies of the X-ray emission from the kpc scale jet in the nearest active galaxy, Cen A. 41 compact sources were found within the jet, 13 of which were newly identified. We construct the luminosity function for the…