Dust and gas environment of the young embedded cluster IRAS 18511+0146

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Table 4

Comparison of properties of cluster members: S7, S10, and S11.

Property	S7	S10	S11

H₂O maser^a	Y	...	...
CH₃OH Class I Maser^b	Y	N	N
CH₃OH Class II Maser^c	Y	...	...
OH Maser^d	N	N	N
Radio detection^e	Y (α< 0.87)	N	Y (α ~ 0.58 ± 0.41)
Bol. luminosity (L_⊙)	≳ 10⁴	...	~ 6000 ^f

Notes. Y – Detection; N – Non-detection; ... – No data available.

^(a)

Urquhart et al. (2011), Beamsize ~ 30′′.

^(b)

Kurtz et al. (2004), Gómez-Ruiz et al. (2016), Synthesized Beam ~2.̋0 × 1.̋4.

^(c)

Fontani et al. (2010), Beamsize ~ 120′′.

^(d)

Edris et al. (2007), Beamsize ~ 3.5′ × 19′.

^(e)

α – Spectral Index (Sánchez-Monge et al. 2011).

^(f)

Based on assumption of optically thin radio emission from a spherical ionised gas distribution.

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