Influence of velocity dispersions on star-formation activities in galaxies

Open Access

Table 1.

Galaxy information.

Project code	Galaxy	Morphology ^(a)	Inclination angle	Distance ^(a)	ALMA array type
			(Degree)	(Mpc)
(1)	(2)	(3)	(4)	(5)	(6)
2013.1.00532.S	NGC628	SA(s)c	6 ^(b)	10.2	12m+ACA+TP
2012.1.01004.S	NGC1808	(R)SAB(s)	57 ^(c)	9.08	12m+ACA+TP
2012.1.00759.S	NGC4568	SA(rs)bc	66 ^(d)	17.3	12m
2013.1.00247.S	Circinus galaxy	SA(s)b	40 ^(e)	4.21	12m+TP
2015.1.01538.S	NGC3627	SAB(s)b	65 ^(f)	9.04	12m
2015.1.01135.S	NGC1365	SB(s)b	46 ^(g)	17.5	12m

Notes. This table presents (1) ALMA project code, (2) name, (3) identified morphology, (4) inclination angle, (5) luminosity distance toward us, (6) array configuration.

References.

^(a)

The informations are obtained from NED.

^(b)

Shostak & van der Kruit (1984).

^(c)

Reif et al. (1982).

^(d)

Vollmer et al. (2013).

^(e)

Chemin et al. (2003).

^(f)

Elmouttie et al. (1998).

^(g)

Ondrechen & van der Hulst (1989).

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.