IRAS 05436-0007 and the Emergence of McNeil's Nebula

Details IRAS 05436-0007 and the Emergence of McNeil's Nebula IRAS 05436-0007 and the Emergence of McNeil's Nebula

2004-03-29

arxiv.org/abs/astro-ph/0403667v1

Astrophys.J. 606 (2004) L119-122

Astronomy and Astrophysics

Astrophysics

9 pages, 5 figures

Scientific paper

10.1086/421393

We present a study of McNeil's Nebula, a newly appeared reflection nebula in the L1630 cloud, together with photometry and spectroscopy of its source. New IR photometry compared to earlier 2MASS data shows that the star has brightened by about 3 magnitudes in the near-infrared, changing its location in a J-H/H-K diagram precisely along a reddening vector. A Gemini NIRI K-band spectrum shows strong CO-bandhead emission and Br-gamma is in emission, indicative of strong accretion. A Gemini GMOS optical spectrum shows only a red, heavily veiled continuum, with H-alpha strongly in emission and displaying a pronounced P Cygni profile, with an absorption trough reaching velocities up to 600 km s-1. This implies significant mass loss in a powerful wind. However, no evidence is found for any shocks, as commonly seen in collimated outflows from young stars. Apparently the eruption has dispersed a layer of extinction and this, together with the intrinsic brightening of the IRAS source, has allowed an earlier outflow cavity to be flooded with light, thus creating McNeil's Nebula.

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