Rotating toroids in G10.62–0.38, G19.61–0.23, and G29.96–0.02

Free Access

Table 1

Phase centers, distances, luminosities, and LSR velocities of the sources.

		Position^a

		α(J2000)	δ(J2000)	L _bol^b	V _LSR	d
Core	IRAS PSC name	h m s	° ′ ″	(L_⊙)	(km s^-1)	(kpc)	Refs.^c


G10.62−0.38	18075−1956	18 10 28.650	−19 55 49.50	0.4 × 10⁶	−2.0	3.4	1
G19.61−0.23	18248−1158	18 27 38.145	−11 56 38.49	2.2 × 10⁶	41.6	12.6	2
G29.96−0.02	18434−0242	18 46 03.955	−02 39 21.87	3.2 × 10⁵	98.9	3.5	3

Notes.

^(a)

Coordinates of the phase center of the observations.

^(b)

Bolometric luminosities calculated by integrating the IRAS flux densities. The contribution from longer wavelengths was taken into account by extrapolating according to a black-body function that peaks at 100 μm and has the same flux density as the source at this wavelength.

^(c)

References for the distances: 1: Blum et al. (2001); 2: Kolpak et al. (2003); 3: L. Moscadelli (2010, priv. comm.).

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.