SPY - the ESO Supernovae type Ia Progenitor survey

Napiwotzki, R., Christlieb, N., Drechsel, H., Hagen, H.J., Heber, U., Homeier, D., Karl, C., Koester, D., Leibundgut, B., Marsh, T.R., Moehler, S., Nelemans, G., Pauli, E.M., Reimers, D., Renzini, A. and Yungelson, L. (2003) SPY - the ESO Supernovae type Ia Progenitor survey. pp. 25-30.

Copy

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.

Item Type	Article
Divisions	?? sbu_spam ?? ?? sbu_specs ?? ?? dep_pam ??
Date Deposited	18 Nov 2024 12:29
Last Modified	18 Nov 2024 12:29

[error in script]

picture_as_pdf

picture_as_pdf: 101258.pdf
: Available under Creative Commons: 4.0

View

Download

Atom

BibTeX

OpenURL ContextObject in Span

OpenURL ContextObject

Dublin Core

MPEG-21 DIDL

EndNote

HTML Citation

METS

MODS

RIOXX2 XML

Reference Manager

Refer

ASCII Citation

Export

Downloads