2008ApJ...678L..55B


Query : 2008ApJ...678L..55B

2008ApJ...678L..55B - Astrophys. J., 678, L55-L58 (2008/May-1)

High spatial resolution spectroscopy of W51 IRS 2E and IRS 2W: two very massive young stars in early formation stages.

BARBOSA C.L., BLUM R.D., CONTI P.S., DAMINELI A. and FIGUEREDO E.

Abstract (from CDS):

We present K-band spectra of the near infrared counterparts to IRS 2E and IRS 2W which is associated with the ultracompact H II region W51d, both of them embedded sources in the Galactic compact H II region W51 IRS 2. The high spatial resolution observations were obtained with the laser guide star facility and Near-infrared Integral Field Spectrograph (NIFS) mounted at the Gemini-North observatory. The spectrum of the ionizing source of W51d shows the photospheric features N III (21155 Å) in emission and He II (21897 Å) in absorption which lead us to classify it as a young O3 type star. We detected CO overtone in emission at 23000 Å in the spectrum of IRS 2E, suggesting that it is a massive young object still surrounded by an accretion disk, probably transitioning from the hot core phase to an ultracompact H II region.

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Journal keyword(s): Infrared: Stars - Stars: Early-Type - Stars: Formation - Techniques: Spectroscopic

Nomenclature: Fig.1: BBCDF N (Nos 1-4).

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 3576 HII 11 11 53.2 -61 18 26           ~ 245 2
2 [WBN74] W 51 IRS 2W Y*O 19 23 39.787 +14 31 07.46           ~ 18 0
3 [WBN74] W 51 IRS 2 SFR 19 23 39.93 +14 31 09.4           ~ 321 0
4 NAME W 51 North Rad 19 23 40.0 +14 30 51           ~ 169 0
5 [WBN74] W 51 IRS 2E Y*O 19 23 40.167 +14 31 06.63           ~ 24 0
6 OKYM 2 IR 19 23 40.26 +14 31 06.6           ~ 5 0
7 NAME W 51 IRS 1 HII 19 23 41.9 +14 30 36           ~ 124 0
8 NAME W 51 Main reg 19 23 43.8 +14 30 37           ~ 147 0
9 W 51 SNR 19 23 50 +14 06.0           ~ 1352 1
10 HD 189920 * 20 02 04.9379961264 +12 19 19.548231564   9.42 9.36     A0V 22 0

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