- Open Access
Erratum to: Thermal and hydrostatic structure of the protoplanetary nebula exposed to stellar radiation and stellar wind from the central star
- Young Seok Yun,
- Hiroyuki Emori and
- Kiyoshi Nakazawa
© The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences; TERRAPUB 2010
- Published: 13 February 2015
The original article was published in Earth, Planets and Space 2007 59:BF03352724
Section 2. Equation (10): “P = f P w at z = z s ,” should be replaced by “P = f2 P w at z = z s ,”.
Fortunately, the results on the temperature distribution and the height of the nebula hardly change even if the equations change. However, the behavior of solutions near the critical point changes. As a result, there exist surely the steady state solutions of the nebula, even if the wind parameter, t*/β, is smallar than 1 × 107 yr although the above-mentioned paper declared that there is no solution in such an extremely strong wind case.