The role of molecular gas in the nuclear regions of IRAS 00183-7111 - ALMA and X-ray investigations of an ultraluminous infrared galaxy

Home

All issues

Volume 616 (August 2018)

A&A, 616 (2018) A127

Full HTML

Free Access

Table 3.

ALMA continuum emission properties.

	Freq. ranges^a (GHz)	Flux density^b (mJy)	rms^c (mJy beam⁻¹)	Beam size^d (″)	Source size^e (kpc²)	Luminosity^f (erg s⁻¹)
Band 3	86.1–87.8/96.2–97.7	3.4 ± 0.3	0.016	3.01 × 2.05	(3.37 ± 0.2) × (2.26 ± 0.1)	~8.2 × 10⁴¹
Band 6	257.2–259.11/272.35–274.22	2.2 ± 0.2	0.015	2.35 × 1.19	(4.8 ± 1.1) × (3.8 ± 1)	~2.1 × 10⁴²
	253.3–255.2/266.2–267.8	2.6 ± 0.3	0.05	2.48 × 1.31	(3.9 ± 0.8) × (2.7 ± 0.52)	~2.4 × 10⁴²

Notes.

^(a)

Observed frequency ranges.

^(b)

Integrated continuum flux density.

^(c)

1σ rms noise level, measured in source-free regions.

^(d)

Synthesized beam sizes of natural weighted continuum maps.

^(e)

Source spatial extent deconvolved from the clean beam.

^(f)

Luminosity associated with the continuum emission in each band.

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.