Header

UZH-Logo

Maintenance Infos

Forming a large disc galaxy from a z < 1 major merger


Governato, F; Brook, C B; Brooks, A M; Mayer, L; Willman, B; Jonsson, P; Stilp, A M; Pope, L; Christensen, C; Wadsley, J; Quinn, T (2009). Forming a large disc galaxy from a z < 1 major merger. Monthly Notices of the Royal Astronomical Society, 398(1):312-320.

Abstract

Using high-resolution SPH simulations in a fully cosmological Λ cold dark matter context, we study the formation of a bright disc-dominated galaxy that originates from a 'wet' major merger at z= 0.8 . The progenitors of the disc galaxy are themselves disc galaxies that formed from early major mergers between galaxies with blue colours. A substantial thin stellar disc grows rapidly following the last major merger and the present-day properties of the final remnant are typical of early-type spiral galaxies, with an i-band bulge-to-disc ratio ∼0.65, a disc scalelength of 7.2 kpc, g−r= 0.5 mag , an H i linewidth (W20/2) of 238 km s−1 and total magnitude i=−22.4 . The key ingredients for the formation of a dominant stellar disc component after a major merger are (i) substantial and rapid accretion of gas through cold flows followed at late times by cooling of gas from the hot phase, (ii) supernova feedback that is able to partially suppress star formation during mergers and (iii) relative fading of the spheroidal component. The gas fraction of the progenitors' discs does not exceed 25 per cent at z < 3 , emphasizing that the continuous supply of gas from the local environment plays a major role in the regrowth of discs and in keeping the galaxies blue. The results of this simulation alleviate the problem posed for the existence of disc galaxies by the high likelihood of interactions and mergers for galaxy-sized haloes at relatively low z.

Abstract

Using high-resolution SPH simulations in a fully cosmological Λ cold dark matter context, we study the formation of a bright disc-dominated galaxy that originates from a 'wet' major merger at z= 0.8 . The progenitors of the disc galaxy are themselves disc galaxies that formed from early major mergers between galaxies with blue colours. A substantial thin stellar disc grows rapidly following the last major merger and the present-day properties of the final remnant are typical of early-type spiral galaxies, with an i-band bulge-to-disc ratio ∼0.65, a disc scalelength of 7.2 kpc, g−r= 0.5 mag , an H i linewidth (W20/2) of 238 km s−1 and total magnitude i=−22.4 . The key ingredients for the formation of a dominant stellar disc component after a major merger are (i) substantial and rapid accretion of gas through cold flows followed at late times by cooling of gas from the hot phase, (ii) supernova feedback that is able to partially suppress star formation during mergers and (iii) relative fading of the spheroidal component. The gas fraction of the progenitors' discs does not exceed 25 per cent at z < 3 , emphasizing that the continuous supply of gas from the local environment plays a major role in the regrowth of discs and in keeping the galaxies blue. The results of this simulation alleviate the problem posed for the existence of disc galaxies by the high likelihood of interactions and mergers for galaxy-sized haloes at relatively low z.

Statistics

Citations

Dimensions.ai Metrics
152 citations in Web of Science®
141 citations in Scopus®
202 citations in Microsoft Academic
Google Scholar™

Altmetrics

Downloads

120 downloads since deposited on 25 Feb 2010
15 downloads since 12 months
Detailed statistics

Additional indexing

Item Type:Journal Article, refereed, original work
Communities & Collections:07 Faculty of Science > Institute for Computational Science
Dewey Decimal Classification:530 Physics
Language:English
Date:2009
Deposited On:25 Feb 2010 20:00
Last Modified:31 Jul 2018 15:22
Publisher:Wiley-Blackwell
ISSN:0035-8711
Additional Information:The definitive version is available at www.blackwell-synergy.com
OA Status:Green
Publisher DOI:https://doi.org/10.1111/j.1365-2966.2009.15143.x
Related URLs:http://arxiv.org/abs/0812.0379

Download

Download PDF  'Forming a large disc galaxy from a z < 1 major merger'.
Preview
Content: Accepted Version
Language: English
Filetype: PDF (Accepted manuscript, Version 2)
Size: 1MB
View at publisher
Download PDF  'Forming a large disc galaxy from a z < 1 major merger'.
Preview
Content: Accepted Version
Language: English
Filetype: PDF (Accepted manuscript, Version 1)
Size: 447kB
Download PDF  'Forming a large disc galaxy from a z < 1 major merger'.
Preview
Content: Published Version
Language: English
Filetype: PDF (Nationallizenz 142-005)
Size: 7MB