Loading…

JWST reveals a possible \(z \sim 11\) galaxy merger in triply-lensed MACS0647\(-\)JD

MACS0647\(-\)JD is a triply-lensed \(z\sim11\) galaxy originally discovered with the Hubble Space Telescope. Here we report new JWST imaging, which clearly resolves MACS0647\(-\)JD as having two components that are either merging galaxies or stellar complexes within a single galaxy. Both are very sm...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2023-05
Main Authors: Tiger Yu-Yang Hsiao, Coe, Dan, Abdurro'uf, Whitler, Lily, Jung, Intae, Khullar, Gourav, Meena, Ashish Kumar, Dayal, Pratika, Barrow, Kirk S S, Santos-Olmsted, Lillian, Casselman, Adam, Vanzella, Eros, Nonino, Mario, Jimenez-Teja, Yolanda, Oguri, Masamune, Stark, Daniel P, Furtak, Lukas J, Zitrin, Adi, Adamo, Angela, Brammer, Gabriel, Bradley, Larry, Diego, Jose M, Zackrisson, Erik, Finkelstein, Steven L, Windhorst, Rogier A, Bhatawdekar, Rachana, Hutchison, Taylor A, Broadhurst, Tom, Dimauro, Paola, Andrade-Santos, Felipe, Eldridge, Jan J, Acebron, Ana, Avila, Roberto J, Bayliss, Matthew B, Benitez, Alex, Binggeli, Christian, Bolan, Patricia, Bradac, Marusa, Carnall, Adam C, Conselice, Christopher J, Donahue, Megan, Frye, Brenda, Fujimoto, Seiji, Henry, Alaina, James, Bethan L, Kassin, Susan, Kewley, Lisa, Larson, Rebecca L, Lauer, Tod, Law, David, Mahler, Guillaume, Mainali, Ramesh, McCandliss, Stephan, Nicholls, David, Pirzkal, Norbert, Postman, Marc, Rigby, Jane R, Ryan, Russell, Senchyna, Peter, Keren, Sharon, Shimizu, Ikko, Strait, Victoria, Tang, Mengtao, Trenti, Michele, Vikaeus, Anton, Welch, Brian
Format: Article
Language:English
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:MACS0647\(-\)JD is a triply-lensed \(z\sim11\) galaxy originally discovered with the Hubble Space Telescope. Here we report new JWST imaging, which clearly resolves MACS0647\(-\)JD as having two components that are either merging galaxies or stellar complexes within a single galaxy. Both are very small, with stellar masses \(\sim10^8\,M_\odot\) and radii \(r
ISSN:2331-8422
DOI:10.48550/arxiv.2210.14123