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相关论文: Masses of Isolated Spiral KIG Galaxies

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We use the data of modern digital sky surveys (PanSTARRS-1, SDSS) combined with HI-line and far ultraviolet (GALEX) surveys to reclassify 165 early-type galaxies from the Catalog of Isolated Galaxies (KIG). As a result, the number of E- and…

星系天体物理 · 物理学 2021-12-22 V. E. Karachentseva , I. D. Karachentsev , O. V. Melnyk

We present the results of a search for companions around the isolated galaxies from the 2MIG catalog. Among 3227 2MIG galaxies we detected 125 objects with a total of 214 neighbors having radial velocity differences of Delta V < 500 km/s…

宇宙学与河外天体物理 · 物理学 2015-06-03 V. E. Karachentseva , I. D. Karachentsev , O. V. Melnyk

Rapid advance has been made recently in accurate distance measurements for nearby ($D < 11$ Mpc) galaxies based on the magnitude of the tip of red giant branch stars resolved with the Hubble Space Telescope. We use observational properties…

星系天体物理 · 物理学 2021-09-02 Igor D. Karachentsev , Olga G. Kashibadze

We use a sample of 220 face-on bulge-less galaxies situated in the low density environment to estimate their total mass via orbital motions of supposed rare satellites. Our inspection reveals 43 dwarf companions having the mean projected…

星系天体物理 · 物理学 2019-05-08 I. D. Karachentsev , V. E. Karachentseva

We present a revised and expanded catalog of satellite galaxies of a set of isolated spiral galaxies similar in luminosity to the Milky Way. This sample of 115 satellites, 69 of which were discovered in our multifiber redshift survey, is…

天体物理学 · 物理学 2009-09-25 Dennis Zaritsky , Rodney Smith , Carlos Frenk , Simon D. M. White

The radial velocities are measured for 45 galaxies located in the neighborhoods of 29 likely isolated galaxies in a new catalog. We find that about 85% of these galaxies actually are well isolated objects. 4% of nearby galaxies with…

宇宙学与河外天体物理 · 物理学 2015-05-13 O. V. Melnyk , V. E. Karachentseva , I. D. Karachentsev , D. I. Makarov , I. V. Chilingarian

We present a list of 75 isolated late-type dwarf galaxies which have no neighbors with a relative radial velocity difference of less than 500 km/s or projected separations within 500 kpc. These were selected from $\sim$2000 dwarf galaxies…

宇宙学与河外天体物理 · 物理学 2011-04-14 V. E. Karachentseva , I. D. Karachentsev , M. E. Sharina

We estimated the dynamical masses of 115 early-type galaxies (ETGs) by analyzing the dynamics of satellite and companion galaxies of these ETGs. We selected galaxies with absolute magnitudes between -22 and -25 in the $K_s$-band from the…

星系天体物理 · 物理学 2020-11-04 Cheng-Yu Chen , Chorng-Yuan Hwang

We present a complete POSS II-based refinement of the optical morphologies for galaxies in the Karatchenseva's Catalog of Isolated Galaxies that forms the basis of the AMIGA project. Comparison with independent classifications made for an…

We consider seven distant galaxies with clearly evident spiral structure from HST images. Three of these were chosen from Vogt et al. (1996) (VFP) and have measured rotational velocities. Five were chosen from the Medium Deep Survey and are…

天体物理学 · 物理学 2009-10-30 A. C. Quillen , V. L. Sarajedini

We aim to identify and quantify the effects of the satellite distribution around a sample of galaxies in the Catalogue of Isolated Galaxies (CIG), as well as the effects of the Large Scale Structure (LSS) using the SDSS-DR9. To recover the…

We present a catalog of 520 most isolated nearby galaxies with radial velocities V_LG<3500 km/s covering the entire sky. This population of "space orphans" makes up 4.8% among 10900 galaxies with measured radial velocities. We describe the…

宇宙学与河外天体物理 · 物理学 2011-03-23 I. D. Karachentsev , D. I. Makarov , V. E. Karachentseva , O. V. Melnyk

We analyse the properties of a sample of 22 bright isolated spiral galaxies on the basis of Johnson B,V,I images and optical rotation curves. The fraction of early morphological types in our sample of isolated galaxies (or in other samples…

天体物理学 · 物理学 2007-05-23 I. Marquez , M. Moles

The 2MFGC catalog we have used contains 18020 galaxies selected from the extended objects in the 2MASS infrared sky survey as having apparent ratios of the axes b/a<0.3. Most of them are spiral galaxies of later morphological types whose…

天体物理学 · 物理学 2008-11-26 I. D. Karachentsev , Yu. N. Kudrya , V. E. Karachentseva , S. N. Mitronova

We undertook searches for isolated galaxies based on automatic selection of infrared sources from the Two Micron All-Sky Survey (2MASS) followed by a visual inspection of their surrounding. Using a modified criterion by Karachentseva…

宇宙学与河外天体物理 · 物理学 2009-08-12 V. E. Karachentseva , S. N. Mitronova , O. V. Melnyk , I. D. Karachentsev

In order to understand nature of building blocks of galaxies in the early universe, we investigate "genuine irregular galaxies (GIGs)" in the nearby universe. Here, GIGs are defined as isolated galaxies without regular structures (spheroid,…

Isolated galaxies are important since they probe the lowest density regimes inhabited by galaxies. We define a sample of 36 nearby isolated early-type galaxies for further study. Our isolation criteria require them to have no…

天体物理学 · 物理学 2009-11-10 Fatma M. Reda , Duncan A. Forbes , Michael A. Beasley , Ewan J. O'Sullivan , Paul Goudfrooij

We use observational properties of galaxies accumulated in the Updated Nearby Galaxy Catalog to derive a dark matter mass of luminous galaxies via motions of their companions. The data on orbital-to-stellar mass ratio are presented for 15…

星系天体物理 · 物理学 2015-06-19 Igor D. Karachentsev , Yuri N. Kudrya

We analyze empirical relationships between the optical, near infrared, and HI characteristics of isolated galaxies from the 2MIG Catalog covering the entire sky. Data on morphological types, K_S-, and B-magnitudes, linear diameters, HI…

宇宙学与河外天体物理 · 物理学 2015-06-03 Yu. N. Kudrya , V. E. Karachentseva , I. D. Karachentsev

We identify a large sample of isolated bright galaxies and their fainter satellites in the 2dF Galaxy Redshift Survey (2dFGRS). We analyse the dynamics of ensembles of these galaxies selected according to luminosity and morphological type…

天体物理学 · 物理学 2009-11-13 Peder Norberg , Carlos S. Frenk , Shaun Cole
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