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We observed the nearest gravitational lensing cluster candidate, A 3408 (${\it z}=0.042$), with ASCA. The projected mass profile of A 3408 was determined from the ICM temperature and the $\beta$-model parameters obtained with ASCA, assuming…

天体物理学 · 物理学 2015-06-24 Haruyoshi Katayama , Kiyoshi Hayashida , Kiyoshi Hashimotodani

We present Atacama Large Millimeter/submillimeter Array observations of a radio-loud and millimeter-bright galaxy at z=2.6. Gravitational lensing by a foreground galaxy at z~0.2 provides access to physical scales of approximately 360 pc,…

星系天体物理 · 物理学 2018-10-24 J. E. Geach , R. J. Ivison , S. Dye , I. Oteo

Omega Centauri ($\omega\,$Cen) is the most massive and chemically complex star cluster in the Milky Way and is widely regarded as the surviving nuclear star cluster of an accreted dwarf galaxy. However, its parent host remains uncertain.…

We present the first census of giant molecular clouds (GMCs) complete down to 10$^6 M_{\odot}$ and within the inner 4 kpc of the nearest giant elliptical and powerful radio galaxy, Centaurus A. We identified 689 GMCs using CO(1--0) data…

Convincing evidence of a past interaction between two rich clusters A399 and A401 was recently found by the X-ray imaging observations. In this paper we examine the structure and dynamics of this pair of galaxy clusters. A mixture-modeling…

天体物理学 · 物理学 2009-11-10 Qirong Yuan , Pengfei Yan , Yanbin Yang , Xu Zhou

Aims: We present the first measurement of the proper motion and orbit of the very distant and intriguing globular cluster NCG 2419. Methods: We have combined data from HST and Gaia DR1 to derive the relative proper motions of stars in the…

星系天体物理 · 物理学 2017-02-22 Davide Massari , Lorenzo Posti , Amina Helmi , Giuliana Fiorentino , Eline Tolstoy

Alpha Centauri is a triple stellar system, and it contains the closest star to Earth (Proxima Centauri). Over the last decades, the stars in Alpha Cen and their orbits have been investigated in great detail. However, the possible scenarios…

地球与行星天体物理 · 物理学 2024-01-30 Nicolás Cuello , Mario Sucerquia

A major uncertainty in the dynamical history of the local group of galaxies originates from the unknown transverse speed of the Andromeda galaxy (M31) relative to the Milky Way. We show that the recent VLBA measurement of the proper motion…

天体物理学 · 物理学 2009-11-13 Abraham Loeb , Mark J. Reid , Andreas Brunthaler , Heino Falcke

Thanks to modern sky surveys, over twenty stellar streams and overdensity structures have been discovered in the halo of the Milky Way. In this paper, we present an analysis of spectroscopic observations of individual stars from one such…

Our Galaxy and the nearby Andromeda Galaxy (M31) form a bound system, even though the relative velocity vector of M31 is currently not well constrained. Their orbital motion is highly dependent on the initial conditions, but all the…

星系天体物理 · 物理学 2020-03-18 Riccardo Schiavi , Roberto Capuzzo Dolcetta , Manuel Arca Sedda , Mario Spera

The bright, nearby binary $\alpha$ Centauri provides an excellent laboratory for testing stellar evolution models, as it is one of the few stellar systems for which we have high-precision classical (mass, radius, luminosity) and…

太阳与恒星天体物理 · 物理学 2018-09-19 M. Joyce , B. Chaboyer

We present an all-sky catalogue of 395 nearby galaxy groups revealed in the Local Supercluster and its surroundings. The groups and their associations are identified among 10914 galaxies at |b|>15deg with radial velocities VLG<3500 km/s.…

宇宙学与河外天体物理 · 物理学 2015-05-20 Dmitry Makarov , Igor Karachentsev

Our Galaxy, Andromeda and their companion dwarf galaxies form the Local Group. Most of the mass in and around it is believed to be dark matter rather than gas or stars, so its distribution must be inferred from the effect of gravity on the…

星系天体物理 · 物理学 2026-01-27 Ewoud Wempe , Simon D. M. White , Amina Helmi , Guilhem Lavaux , Jens Jasche

We place constraints on the dynamics of the Local Group (LG) by comparing the dipole of the Cosmic Microwave Background (CMB) with the peculiar velocity induced by the 2MRS galaxy sample. The analysis is limited by the lack of surveyed…

天体物理学 · 物理学 2009-11-13 Abraham Loeb , Ramesh Narayan

The physical state of the gas in the central 500 pc of NGC~5128 (the radio galaxy Centaurus A - Cen A), was investigated using the far-infrared fine-structure lines of carbon, oxygen, and nitrogen, as well as the CO(4-3) molecular line. The…

星系天体物理 · 物理学 2017-03-01 F. P. Israel , R. Guesten , R. Meijerink , M. A. Requena-Torres , J. Stutzki

We present deep GALEX images of NGC 5128, the parent galaxy of Centaurus A. We detect a striking "weather ribbon" of Far-UV and H$\alpha$ emission, which extends more than 35 kpc northeast of the galaxy. The ribbon is associated with a…

星系天体物理 · 物理学 2015-06-23 Susan G. Neff , Jean A. Eilek , Frazer N. Owen

We use data from the ESA Gaia mission Early Data Release 3 (EDR3) to measure the trigonometric parallax of $\omega$ Cen, the first high precision parallax measurement for the most massive globular cluster in the Milky Way. We use a…

星系天体物理 · 物理学 2021-02-12 John Soltis , Stefano Casertano , Adam G. Riess

Aims. 2015 BZ509 is the first asteroid confirmed to be in retrograde co-orbit resonance (or 1/-1 resonance) with the giant planets in the solar system. While Saturn is the only giant planet whose Trojans are not discovered until now, we…

地球与行星天体物理 · 物理学 2018-10-03 Miao Li , Yukun Huang , Shengping Gong

We report trigonometric parallax measurements of masers in the massive star forming complex W43 from VLBA observations as part of the BeSSeL Survey. Based on measurements of three 12 GHz methanol maser sources (G029.86-00.04, G029.95-00.01…

星系天体物理 · 物理学 2015-06-18 B. Zhang , L. Moscadelli , M. Sato , M. J. Reid , K. M. Menten , X. W. Zheng , A. Brunthaler , T. M. Dame , Y. Xu , K. Immer

The spherical infall model first developed by Lema\^{i}tre and Tolman was modified in order to include the effects of a dark energy term. The resulting velocity-distance relation was evaluated numerically. This equation, when fitted to…

天体物理学 · 物理学 2016-08-16 Sébastien Peirani , José Antonio De Freitas Pacheco