Convective overshooting and the observed width of the main-sequence band

R. Napiwotzki; A. Rieschick; T. Blocker; D. Schonberner; V. Wenske

Convective overshooting and the observed width of the main-sequence band

R. Napiwotzki, A. Rieschick, T. Blocker, D. Schonberner, V. Wenske

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Abstract

For many years we are witnessing a lively debate on the existence and extent of convective overshooting, mainly in the cores of main-sequence stars. This is an important issue, since even a small amount of overshooting increases considerably the mass of the finally hydrogen exhausted core and lengthens the main-sequence lifetime correspondingly.

Original language	English
Title of host publication	In: Procs Inside the Stars, IAU Colloquium 137
Publisher	Astronomical Society of the Pacific
Pages	461-463
ISBN (Print)	0-937707-59-7
Publication status	Published - 1993

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title = "Convective overshooting and the observed width of the main-sequence band",

abstract = "For many years we are witnessing a lively debate on the existence and extent of convective overshooting, mainly in the cores of main-sequence stars. This is an important issue, since even a small amount of overshooting increases considerably the mass of the finally hydrogen exhausted core and lengthens the main-sequence lifetime correspondingly.",

author = "R. Napiwotzki and A. Rieschick and T. Blocker and D. Schonberner and V. Wenske",

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year = "1993",

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T1 - Convective overshooting and the observed width of the main-sequence band

AU - Napiwotzki, R.

AU - Rieschick, A.

AU - Blocker, T.

AU - Schonberner, D.

AU - Wenske, V.

N1 - Original paper can be found at: http://www.astrosociety.org/pubs/cs/confseries.html#2--Copyright Astronomical Society of the Pacific

PY - 1993

Y1 - 1993

N2 - For many years we are witnessing a lively debate on the existence and extent of convective overshooting, mainly in the cores of main-sequence stars. This is an important issue, since even a small amount of overshooting increases considerably the mass of the finally hydrogen exhausted core and lengthens the main-sequence lifetime correspondingly.

AB - For many years we are witnessing a lively debate on the existence and extent of convective overshooting, mainly in the cores of main-sequence stars. This is an important issue, since even a small amount of overshooting increases considerably the mass of the finally hydrogen exhausted core and lengthens the main-sequence lifetime correspondingly.

M3 - Conference contribution

SN - 0-937707-59-7

SP - 461

EP - 463

BT - In: Procs Inside the Stars, IAU Colloquium 137

PB - Astronomical Society of the Pacific

ER -

Convective overshooting and the observed width of the main-sequence band

Abstract

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