SPY - the ESO Supernovae type Ia Progenitor survey

R. Napiwotzki; N. Christlieb; H. Drechsel; H.J. Hagen; U. Heber; D. Homeier; C. Karl; D. Koester; B. Leibundgut; T.R. Marsh; S. Moehler; G. Nelemans; E.M. Pauli; D. Reimers; A. Renzini; L. Yungelson

SPY - the ESO Supernovae type Ia Progenitor survey

R. Napiwotzki
, N. Christlieb
, H. Drechsel
, H.J. Hagen
, U. Heber
, D. Homeier
, C. Karl
, D. Koester
, B. Leibundgut
, T.R. Marsh
, S. Moehler
, G. Nelemans
, E.M. Pauli
, D. Reimers
, A. Renzini
, L. Yungelson

Research output: Contribution to journal › Article › peer-review

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Abstract

Supernovae (SNe) mark the violent termination of a star’s life in an explosion. They are classified according to their light curve as type I or II, with the type I SNe producing very similar light curves, while the SNe type II are more diverse. Spectroscopic observations reveal the presence of hydrogen in SNe type II, while no hydrogen lines are detectable in SNe type I. According to their spectral appearance the type I class can be further subdivided into Ia, Ib, and Ic.

Original language	English
Pages (from-to)	25-30
Journal	The Messenger
Volume	112
Publication status	Published - 2003

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@article{a7adb5c3310b4a628a1dc07dc3af9784,

title = "SPY - the ESO Supernovae type Ia Progenitor survey",

abstract = "Supernovae (SNe) mark the violent termination of a star{\textquoteright}s life in an explosion. They are classified according to their light curve as type I or II, with the type I SNe producing very similar light curves, while the SNe type II are more diverse. Spectroscopic observations reveal the presence of hydrogen in SNe type II, while no hydrogen lines are detectable in SNe type I. According to their spectral appearance the type I class can be further subdivided into Ia, Ib, and Ic.",

author = "R. Napiwotzki and N. Christlieb and H. Drechsel and H.J. Hagen and U. Heber and D. Homeier and C. Karl and D. Koester and B. Leibundgut and T.R. Marsh and S. Moehler and G. Nelemans and E.M. Pauli and D. Reimers and A. Renzini and L. Yungelson",

note = "Original article can be found at: http://www.eso.org/sci/publications/messenger/",

year = "2003",

language = "English",

volume = "112",

pages = "25--30",

journal = "The Messenger",

}

TY - JOUR

T1 - SPY - the ESO Supernovae type Ia Progenitor survey

AU - Napiwotzki, R.

AU - Christlieb, N.

AU - Drechsel, H.

AU - Hagen, H.J.

AU - Heber, U.

AU - Homeier, D.

AU - Karl, C.

AU - Koester, D.

AU - Leibundgut, B.

AU - Marsh, T.R.

AU - Moehler, S.

AU - Nelemans, G.

AU - Pauli, E.M.

AU - Reimers, D.

AU - Renzini, A.

AU - Yungelson, L.

N1 - Original article can be found at: http://www.eso.org/sci/publications/messenger/

PY - 2003

Y1 - 2003

N2 - Supernovae (SNe) mark the violent termination of a star’s life in an explosion. They are classified according to their light curve as type I or II, with the type I SNe producing very similar light curves, while the SNe type II are more diverse. Spectroscopic observations reveal the presence of hydrogen in SNe type II, while no hydrogen lines are detectable in SNe type I. According to their spectral appearance the type I class can be further subdivided into Ia, Ib, and Ic.

AB - Supernovae (SNe) mark the violent termination of a star’s life in an explosion. They are classified according to their light curve as type I or II, with the type I SNe producing very similar light curves, while the SNe type II are more diverse. Spectroscopic observations reveal the presence of hydrogen in SNe type II, while no hydrogen lines are detectable in SNe type I. According to their spectral appearance the type I class can be further subdivided into Ia, Ib, and Ic.

M3 - Article

VL - 112

SP - 25

EP - 30

JO - The Messenger

JF - The Messenger

ER -

SPY - the ESO Supernovae type Ia Progenitor survey

Abstract

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