Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Hasti Nateghi"'
Autor:
Tania M. Barone, Glenn G. Kacprzak, James W. Nightingale, Nikole M. Nielsen, Karl Glazebrook, Kim-Vy H. Tran, Tucker Jones, Hasti Nateghi, Keerthi Vasan Gopala Chandrasekaran, Nandini Sahu, Themiya Nanayakkara, Hannah Skobe, Jesse van de Sande, Sebastian Lopez, Geraint F. Lewis
Publikováno v:
Communications Physics, Vol 7, Iss 1, Pp 1-11 (2024)
Abstract While quiescent galaxies have comparable amounts of cool gas in their outer circumgalactic medium (CGM) compared to star-forming galaxies, they have significantly less interstellar gas. However, open questions remain on the processes causing
Externí odkaz:
https://doaj.org/article/b3c92d0089cf4e2e94e32a8a86ae3ab7
Autor:
THEMIYA NANAYAKKARA, Karl Glazebrook, Colin Jacobs, Corentin Schreiber, Gabriel Brammer, James Esdaile, Glenn Kacprzak, Ivo Labbe, Claudia Lagos, Danilo Marchesini, Cemile Marsan, Hasti Nateghi, Pascal Oesch, Casey Papovich, Rhea-Silvia Remus, Kim-Vy Tran
The confirmation of the presence of very massive quiescent galaxies at epochs only 1–2 Gyr after the Big Bang [1–8] has challenged models of cosmology and galaxy formation [9]. Producing sufficient numbers of these requires abundant numbers of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e6a2b4651991b7ccb61d1d098883c454
https://doi.org/10.21203/rs.3.rs-2404918/v1
https://doi.org/10.21203/rs.3.rs-2404918/v1
Autor:
Christopher W. Churchill, Hasti Nateghi, Nikole M. Nielsen, Glenn G. Kacprzak, Jane C. Charlton, S. Muzahid, Stephanie K. Pointon, Themiya Nanayakkara
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 500:2289-2301
The relationship between a galaxy's properties and its circumgalactic medium (CGM) provides a unique view of how galaxies evolve. We present an interesting edge-on (i=86 degrees) disk galaxy (G1547) where the CGM is probed by a background quasar at a
Autor:
Christopher W. Churchill, S. Muzahid, Hasti Nateghi, Nikole M. Nielsen, Glenn G. Kacprzak, Stephanie K. Pointon, Jane C. Charlton
The multi-phase circumgalactic medium (CGM) arises within the complex environment around a galaxy, or collection of galaxies, and possibly originates from a wide range of physical mechanisms. In this paper, we attempt to disentangle the origins of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::955ff94599f136d96669c193a236a7a1
http://arxiv.org/abs/2011.06071
http://arxiv.org/abs/2011.06071
Autor:
Hasti Nateghi
Among the most pressing problems in galaxy formation and evolution is to understand how gas accretion and feedback influence the evolution of galaxies. In order to determine how galaxies evolve, we need to have a firm understanding of structure, kine
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b4bb0493e65d246e1e7a347338ba612
Autor:
Barone, Tania M.1,2,3 tbarone@swin.edu.au, Kacprzak, Glenn G.1,2, Nightingale, James W.4, Nielsen, Nikole M.1,2,5, Glazebrook, Karl1,2, Tran, Kim-Vy H.2,3,6, Jones, Tucker7, Nateghi, Hasti1,2, Vasan Gopala Chandrasekaran, Keerthi7, Sahu, Nandini2,3, Nanayakkara, Themiya1,2, Skobe, Hannah8, van de Sande, Jesse9, Lopez, Sebastian10, Lewis, Geraint F.9
Publikováno v:
Communications Physics. 8/24/2024, Vol. 7 Issue 1, p1-11. 11p.