The molecular gas reservoir of 6 low-metallicity galaxies from the Herschel Dwarf Galaxy Survey - A ground-based follow-up survey of CO(1–0), CO(2–1), and CO(3–2)

D. Cormier; S. C. Madden; V. Lebouteiller; S. Hony; S. Aalto; F. Costagliola; A. Hughes; A. Rémy-Ruyer; N. Abel; E. Bayet; F. Bigiel; J. M. Cannon; R. J. Cumming; M. Galametz; F. Galliano; S. Viti; R. Wu

doi:10.1051/0004-6361/201322096

Home

All issues

Volume 564 (April 2014)

A&A, 564 (2014) A121

Full HTML

Free Access

Table 4

Spitzer/IRS H₂ observations and fluxes.

Galaxy		NGC 625	NGC 625	Haro 11^a
Observing mode		staring	total^b	staring
AORKey		5051904		9007104

Line flux:
	H2 S(0) 28.22μm	<18.4	<27.6	<24.9
	H2 S(1) 17.03μm	10.8 ± 2.6	16.2 ± 3.8	16.8 ± 5.5
	H2 S(2) 12.28μm	6.39 ± 1.40	9.58 ± 2.50	10.1 ± 1.3
	H2 S(3) 9.66μm	–	–	12.1 ± 1.8

Notes. Fluxes are in 10^-18 W m^-2 and upper limits are given at a 3σ level.

^(a)

Estimated total H₂ emission from the galaxy by scaling each flux measured in the IRS slit to the 24μm emission of the galaxy.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.