The ultra-diffuse galaxy NGC 1052-DF2 with MUSE
نویسندگان
چکیده
منابع مشابه
Dense Plasma Torus in the GPS Galaxy NGC 1052
We report results from nearly simultaneous pentachromatic VLBI observations towards a nearby GPS galaxy NGC 1052. The observations at 1.6 and 4.8 GHz with VSOP, and at 2.3, 8.4, and 15.4 GHz with VLBA, provide linear resolutions of ∼ 0.1 pc. Convex spectra of a double-sided jet imply that synchrotron emission is obscured through foreground cold dense plasma, in terms of free–free absorption (FF...
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We have obtained Keck spectra for 16 globular clusters (GCs) associated with the merger remnant elliptical NGC 1052, as well as a long-slit spectrum of the galaxy. We derive ages, metallicities and abundance ratios from simple stellar population models using the methods of Proctor & Sansom (2002), applied to extragalactic GCs for the first time. A number of GCs indicate the presence of strong b...
متن کاملEmission from the Prototypical LINER Galaxy NGC 1052
We examine the 0.1 to 10.0 keV X-ray spectrum of the bright nuclear LINER galaxy NGC 1052, one of two elliptical galaxies known to contain a luminous H2O maser. The observed 2.0 − 10.0 keV spectrum is unusually flat (photon index Γ ∼ 0.2) and best described as intrinsically power-law shaped nuclear flux that is either (1) attenuated by a complex absorber with ∼ 70% of the nuclear flux absorbed ...
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We examine the 0.1 to 10.0 keV X-ray spectrum of the bright nuclear LINER galaxy NGC 1052, one of two elliptical galaxies known to contain a luminous H 2 O maser. The observed 2.0 − 10.0 keV spectrum is unusually flat (photon index Γ ∼ 0.2) and best described as intrinsically power-law shaped nuclear flux that is either (1) attenuated by a complex absorber with ∼ 70% of the nuclear flux absorbe...
متن کاملO maser and a plasma obscuring torus in the radio galaxy NGC 1052
Key words Editorial notes – instruction for authors We present multi-frequency simultaneous VLBA observations at 15, 22 and 43 GHz towards the nucleus of the nearby radio galaxy NGC 1052. These three continuum images reveal a double-sided jet structure, whose relative intensity ratios imply that the jet axis is oriented close to the sky plane. The steeply rising spectra at 15–43 GHz at the inne...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2019
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361/201834909