Diversity of chemistry and excitation conditions in the high-mass star forming complex W33

K. Immer; R. Galván-Madrid; C. König; H. B. Liu; K. M. Menten

doi:10.1051/0004-6361/201423780

Home

All issues

Volume 572 (December 2014)

A&A, 572 (2014) A63

Full HTML

Free Access

Table 3

Pointing center coordinates and rms noise levels of APEX and SMA observations.

			APEX	SMA (230 GHz)
Source^a	RA	Dec	rms_Line	rms_Cont^b	rms_Line
	(hh mm ss.ss)	(dd ′′″″.″)	(mK)	(mK)	(mK)	(mK)
					LSB	USB


W33 Main1	18 14 25.39	−17 54 00.6	13	11	240	330
W33 A1	18 14 36.10	−17 55 03.0	16	9	250	340
W33 B1	18 14 07.07	−18 00 44.7	14	9	250	330
W33 B	18 13 54.33	−18 01 51.7	26	18	240	310
W33 A	18 14 39.00	−17 52 05.0	35	13	150	110
W33 Main	18 14 13.72	−17 55 43.6	31	126	260	350

Notes.

^(a)

In this table and in the rest of this publication, the W33 sources are sorted along the evolutionary sequence that is established in Sects. 5, 6, and 8.

^(b)

The conversion factor from mJy beam^-1 to mK is 1.8.

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.