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A great challenge in present-day physics is to understand whether the observed internal dynamics of galaxies is due to dark matter matter or due to a modification of the law of gravity. Recently, van Dokkum et al. reported that the…

Recent observations of ultra-dwarf galaxy NGC1052-DF2 started an interesting discussion between dark matter hypothesis and modified gravity theories. Reported low velocity dispersion (< 10.5 km/s at 90% confidence level) derived from the…

广义相对论与量子宇宙学 · 物理学 2019-12-10 Tousif Islam , Koushik Dutta

It was recently proposed that the globular cluster system of the very low surface-brightness galaxy NGC1052-DF2 is dynamically very cold, leading to the conclusion that this dwarf galaxy has little or no dark matter. Here, we show that a…

星系天体物理 · 物理学 2018-05-23 Nicolas F. Martin , Michelle L. M. Collins , Nicolas Longeard , Erik Tollerud

The Ultra-Diffuse galaxy NGC1052-DF2 has recently been under intense scrutiny because from its kinematics it has revealed to be "extremely deficient" in dark matter, if not lacking it at all. This claim has raised many questions and…

广义相对论与量子宇宙学 · 物理学 2022-11-09 Enrico Laudato , Vincenzo Salzano

The ultra-diffuse galaxy NGC1052-DF2 has a very low velocity dispersion, indicating that it has little or no dark matter. Here we report the discovery of a second galaxy in this class, residing in the same group. NGC1052-DF4 closely…

星系天体物理 · 物理学 2019-04-03 Pieter van Dokkum , Shany Danieli , Roberto Abraham , Charlie Conroy , Aaron J. Romanowsky

Using ultra-deep imaging ($\mu_g = 30.4$ mag/arcsec$^2$; 3$\sigma$, 10"x10"), we probed the surroundings of the first galaxy "lacking" dark matter KKS2000[04] (NGC 1052-DF2). Signs of tidal stripping in this galaxy would explain its claimed…

星系天体物理 · 物理学 2021-09-29 Mireia Montes , Ignacio Trujillo , Raúl Infante-Sainz , Matteo Monelli , Alejandro S. Borlaff

The existence of long-lived galaxies lacking dark matter represents a challenge to our understanding of how galaxies form. Here, we present evidence that explains the lack of dark matter in one of such galaxies: NGC1052-DF4. Deep optical…

Recently, \cite{vanDokkum2018} have presented an important discovery of an ultra diffuse galaxy, NGC1052-DF2, with a dark matter content significantly less than predicted from its stellar mass alone. The analysis relies on measured radial…

星系天体物理 · 物理学 2019-01-03 Adi Nusser

A number of scenarios have been proposed to explain the low velocity dispersion (and hence possible absence of dark matter) of the low surface brightness galaxies NGC1052-DF2 and NGC1052-DF4. Most of the proposed mechanisms are based on the…

星系天体物理 · 物理学 2024-04-30 Giulia Golini , Mireia Montes , Eleazar R. Carrasco , Javier Román , Ignacio Trujillo

The recently claimed discovery of an ultra-diffuse galaxy lacking dark matter has important implications for alternate theories to dark matter as well as models of galaxy formation within the $\Lambda$CDM context. In this letter, we present…

星系天体物理 · 物理学 2018-11-01 Aditya Chowdhury

Recent observations revealed a mysterious ultra diffuse galaxy, NGC1052-DF2, in the group of a large elliptical galaxy, NGC1052. Compared to expectations from abundance matching models, the dark matter mass contained in NGC1052-DF2 is…

星系天体物理 · 物理学 2018-08-08 Go Ogiya

Based upon the kinematics of ten globular clusters, it has recently been claimed that the ultra-diffuse galaxy, NCD 1052-DF2, lacks a significant quantity of dark matter. Dynamical analyses have generally assumed that this galaxy is…

星系天体物理 · 物理学 2020-01-29 Geraint F. Lewis , Brendon J. Brewer , Zhen Wan

The dwarf galaxy NGC1052-DF2 has recently been identified as potentially lacking dark matter. If correct, this could be a challenge for MOND, which predicts that low surface brightness galaxies should evince large mass discrepancies.…

星系天体物理 · 物理学 2018-08-01 B. Famaey , S. McGaugh , M. Milgrom

The so-called ultra-diffuse galaxy NGC~1052-DF2 was announced to be a galaxy lacking dark matter based on a spectroscopic study of its constituent globular clusters. Here we present the first spectroscopic analysis of the stellar body of…

The conclusion that the diffuse galaxy NGC1052-DF2 is deficient in dark matter depends critically on the distance, as noted in the original publication and subsequent works. The results of our preliminary assessment of the SBF distance have…

星系天体物理 · 物理学 2018-08-10 John P. Blakeslee , Michele Cantiello

While most dwarf galaxies are strongly dark matter dominated, two remarkable objects in the NGC 1052 field, DF2 and DF4, appear to lack dark matter. DF2 and DF4 were recently found to be part of a trail of low luminosity galaxies that…

星系天体物理 · 物理学 2026-03-18 Michael A. Keim , Pieter van Dokkum , Zili Shen , Shany Danieli , Imad Pasha

The NGC 1052 group, and in particular the discovery of two ultra diffuse galaxies with very low internal velocity dispersions, has been the subject of much attention recently. Here we present radial velocities for a sample of 77 globular…

星系天体物理 · 物理学 2019-09-25 Duncan A. Forbes , Adebusola Alabi , Jean P. Brodie , Aaron J. Romanowsky

NGC1052-DF2 was recently discovered as the dark-matter deficient galaxy claimed by van Dokkum et al. (2018a, vD18). However, large uncertainties on its dynamical mass estimate have been pointed out, concerning the paucity of sample,…

星系天体物理 · 物理学 2018-09-12 Kohei Hayashi , Shigeki Inoue

NGC1052-DF4 was found to be the second "galaxy lacking dark matter" in the NGC1052 group, based on its velocity dispersion of $\sigma_{\rm gc}=4.2^{+4.4}_{-2.2}$ km/s as measured from the radial velocities of seven of its globular clusters.…

星系天体物理 · 物理学 2023-09-20 Zili Shen , Pieter van Dokkum , Shany Danieli

Recently van Dokkum et al. (2018b) reported that the galaxy NGC 1052-DF2 (DF2) lacks dark matter if located at $20$ Mpc from Earth. In contrast, DF2 is a dark-matter-dominated dwarf galaxy with a normal globular cluster population if it has…

星系天体物理 · 物理学 2022-03-09 Moritz Haslbauer , Indranil Banik , Pavel Kroupa , Konstantin Grishunin
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