Dark matter in the Central Region of NGC 3256

We investigated the central mass distribution of the luminous infrared galaxy NGC 3256 at a distance of 35 Mpc by using CO(1-0) observations of the Atacama Large Millimeter and sub-millimeter Array (ALMA) and near-IR data of the Two Micron Sky Survey (2MASS). We found that there is a huge amount of...

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Bibliographic Details
Main Authors: Israa Abdulqasim Mohammed Ali, Hwang, Chorng-Yuan, Zamri Zainal Abidin, Plunkett, Adele Laurie
Format: Article
Language:English
Published: Penerbit Universiti Kebangsaan Malaysia 2018
Online Access:http://journalarticle.ukm.my/12129/1/20%20Israa%20Abdulqasim%20Mohammed%20Ali.pdf
http://journalarticle.ukm.my/12129/
http://www.ukm.my/jsm/malay_journals/jilid47bil6_2018/KandunganJilid47Bil6_2018.html
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Institution: Universiti Kebangsaan Malaysia
Language: English