The molecular gas content of blue dwarf galaxies - A collapsing detached molecular system in He 2–10?

Home

All issues

Volume 496 / No 3 (March IV 2009)

A&A, 496 3 (2009) 677-682

Full HTML

Free Access

Table 2:

CO(3-2) intensities, velocities, and velocity dispersions from Gaussian fits to the central positon of the sample of galaxies observed. Errors derived from the Gaussian fits are indicated in parenthesis. The detections at two positions are indicated for He 2-10, at the offset position (20, 20) the parameters for the two lines detected are reported.
Source	$T_{\rm mb}$ (mK)	$V_{\rm lsr}$ (km s^-1)	DV (km s^-1)	Ico (K km s^-1)
NGC 4123	68.	1333. (5)	124. (10)	9.0 (0.6)
NGC 4385	124.	2151. (2)	66. (5)	8.7 (0.6)
NGC 4630	54.	732. (3)	42. (5)	2.4 (0.3)
NGC 4701	66.	689. (3)	46. (7)	3.2 (0.4)
NGC 4713	54.	656. (5)	127. (10)	7.3 (0.6)
NGC 5253	82.	401. (1)	36. (2)	3.1 (0.1)
He2-10
(0, 0)	312.	850. (0.4)	53. (1.)	17.6 (0.3)
(20, 20)	130.	787. (1.7)	52. (4.)	7.2 (0.5)
(20, 20)	113.	933. (1.2)	17. (2.)	2.0 (0.3)
IC 745	-	-	-	-
NGC 4309	-	-	-	-

Source LaTeX | All tables | In the text

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.