30-micron sources in galaxies with different metallicities

Home

All issues

Volume 626 (June 2019)

A&A, 626 (2019) A92

Full HTML

Free Access

Table 7

List of AGB objects from Fig. 13, which are located in the region of 900 K > T_d > 300 K and 33.1 μm > λ_c > 29.7 μm.

Name	Location	T_d	λ_c (30 μm)	F/Cont (30 μm)
		(K)	(μm)
IRAS 18120+4530 ^(a,b)	Milky Way	872 ± 57	33.04 ± 0.69	0.03 ± 0.01
IRAS 04433-7018 ^(a)	LMC	868 ± 78	29.93 ± 0.70	0.19 ± 0.02
OGLE J052242 ^(a,c)	LMC	868 ± 90	29.91 ± 0.99	0.16 ± 0.03
IRAS 16339-0317 ^(a)	Milky Way	848 ± 74	30.53 ± 0.19	0.14 ± 0.02
MSX LMC 1205 ^(a)	LMC	845 ± 62	29.91 ± 0.54	0.08 ± 0.02
MSX LMC 494 ^(a)	LMC	827 ± 64	29.77 ± 0.46	0.15 ± 0.02
MSX SMC 163 ^(a)	SMC	679 ± 31	30.17 ± 0.35	0.14 ± 0.01
IRAS 04188+0122 ^(a)	Milky Way	660 ± 26	29.97 ± 0.26	0.10 ± 0.01
MSX LMC 474 ^(a)	LMC	512 ± 17	29.79 ± 0.08	0.11 ± 0.01
IRAS 18384-3310 ^(d)	Milky Way	495 ± 12	30.52 ± 0.06	0.66 ± 0.01

Notes. The values of the T_d, λ_c, and F/Cont are taken from Tables D.4–D.6. ^(a)The 30 μm feature is weak. ^(b)The 30 μm feature is very weak. ^(c) Full name of object is OGLE J052242.09-691526.2. ^(d)The decline of the 30 μm feature aftermaximum is very slow.

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.