(Q56562819)

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Probing the post-AGB nature of HD 179821

scientific article published in Astronomy and Astrophysics

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Probing the post-AGB nature of HD 179821 (English)

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E. Josselin

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1

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A. Lèbre

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2

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language of work or name

English

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publication date

March 2001

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published in

Astronomy and Astrophysics

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volume

367

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issue

3

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page(s)

826–830

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cites work

Circumstellar envelopes and Asymptotic Giant Branch stars

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reference URL

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21 January 2018

The Detached Dust Shell around the Massive Star HD 179821.

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21 January 2018

The initial mass function and stellar birthrate in the solar neighborhood

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21 January 2018

A study of several F and G supergiant-like stars with infrared excesses as candidates for proto-planetary nebulae

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21 January 2018

Spectroscopic Study of HD 179821 (IRAS 19114+0002): Proto–Planetary Nebula or Supergiant?

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21 January 2018

A consistent explanation for 12C/13C, 7Li, and 3He anomalies in red giant stars

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21 January 2018

Infrared giants vs. supergiants. II. CO observations

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21 January 2018

Dust particle size distributions around oxygen-rich mass-losing red giants

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21 January 2018

The massive post-red supergiants IRC+10420 and HD 179821

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21 January 2018

Mass loss from evolved stars. III. Mass loss rates for fifty stars from CO J = 1-0 observations

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21 January 2018

Proto-Planetary Nebulae

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21 January 2018

OH and H2O observations of cold IRAS stars

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21 January 2018

Photochemistry and molecular ions in oxygen-rich circumstellar envelopes

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21 January 2018

The photodissociation of CO in circumstellar envelopes

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21 January 2018

Dust grains and gas in the circumstellar envelopes around luminous red giant stars

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retrieved

21 January 2018

Identifiers

DOI

10.1051/0004-6361:20000496

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ResearchGate publication ID

240498626

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(Q56562819)

Probing the post-AGB nature of HD 179821

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