ePubs
The open archive for STFC research publications
Home
About ePubs
Content Policies
News
Help
Privacy/Cookies
Contact ePubs
Full Record Details
Persistent URL
http://purl.org/net/epubs/work/10919495
Record Status
Checked
Record Id
10919495
Title
Goods-Herschel: Gas-to-dust mass ratios and CO-TO-H conversion factors in normal and starbursting galaxies at high-z
Contributors
G Magdis
,
D Rigopoulou (STFC Rutherford Appleton Lab.)
,
E Daddi
,
D Elbaz
,
M Sargent
,
H Dannerbauer
,
H Aussel
,
H Hwang
,
M Pannella
,
J Mullaney
,
R Leiton
,
M Dickinson
,
F Walter
,
J Hodge
,
V Charmandaris
,
D Riechers
,
C Carilli
,
D Scott
Abstract
We explore the gas-to-dust mass ratio (M /M ) and the CO luminosity-to-M conversion factor (?) of two well-studied galaxies in the Great Observatories Origins Deep Survey North field that are expected to have different star-forming modes, the starburst GN20 at z = 4.05 and the normal star-forming galaxy BzK-21000 at z = 1.52. Detailed sampling is available for their Rayleigh-Jeans emission via ground-based millimeter (mm) interferometry (1.1-6.6mm) along with Herschel PACS and SPIRE data that probe the peak of their infrared emission. Using the physically motivated Draine \\& Li models, as well as a modified blackbody function, we measure the dust mass (M ) of the sources and find (2.0 × 10) M for GN20 and (8.6 × 10) M for BzK-21000. The addition of mm data reduces the uncertainties of the derived M by a factor of ?2, allowing the use of the local M /M versus metallicity relation to place constraints on the ? values of the two sources. For GN20 we derive a conversion factor of ? < 1.0 M pc(Kkms), consistent with that of local ultra-luminous infrared galaxies, while for BzK-21000 we find a considerably higher value, ? ?4.0 M pc(Kkms), in agreement with an independent kinematic derivation reported previously. The implied star formation efficiency is ?25 L /M for BzK-21000, a factor of ?5-10 lower than that of GN20. The findings for these two sources support the existence of different disk-like and starburst star formation modes in distant galaxies, although a larger sample is required to draw statistically robust results. © 2011. The American Astronomical Society. All rights reserved.
Organisation
STFC
,
RALSP
,
RALSP - SPD
Keywords
Funding Information
Related Research Object(s):
Licence Information:
Language
English (EN)
Type
Details
URI(s)
Local file(s)
Year
Journal Article
Astrophysical Journal Letters 740 (2011): L15.
doi:10.1088/2041-8205/740/1/L15
2011
Showing record 1 of 1
Recent Additions
Browse Organisations
Browse Journals/Series
Login to add & manage publications and access information for OA publishing
Username:
Password:
Useful Links
Chadwick & RAL Libraries
SHERPA FACT
SHERPA RoMEO
SHERPA JULIET
Journal Checker Tool
Google Scholar