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- W2994726348 abstract "K'-band imaging of the Rosette giant molecular cloud CO emission peak reveals the presence of a newly discovered small cluster of stars, coincident with the IRAS source 06314 + 0427 (Block et al. 1993). We have obtained a high-resolution K-band spectrum of the brightest member of the cluster (dubbed BG/IRS1). The Brγ 2.166 μm line shows a double peaked emission, indicative of a hot star with a disk-like circumstellar geometry. We have obtained JHK photometry, which has allowed us to determine the near-IR extinction toward the cluster (A K = 1. m 5 ±.5). Assuming a distance of 1600 pc for the cluster, we show that at least two of the stars appear to be well above the ZAMS, based upon their inferred spectral types and M K magnitudes. From this we conclude that we are seeing a pre-main-sequence cluster of stars" @default.
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- W2994726348 date "1993-05-01" @default.
- W2994726348 modified "2023-09-23" @default.
- W2994726348 title "On the nature of the stellar cluster at the Rosette GMC CO peak." @default.
- W2994726348 hasPublicationYear "1993" @default.
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