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Projets Spectroscopie

"new stars" spectra

 

Retour Accueil

 

 

 

Main features for "new" stars spectroscopic identification near maximum light

 

Dwarf Novae

 

 

 

WZ Sge type

Intense blue continuum
Balmer lines weak in absorption or emission - sometimes : weak emission component in the absorption component

 

 

 

 

 

VSX J213806.5+261957 | 15-05-2010
(note the emission component in H béta absorption)

Novae
 

 

Type Fe Nova

Narrow lines < 2500 km.s-1
Fe lines especially multiplet 42
Frequent P Cygni absorption profile

Slow evolution (weeks)

 

V496 Sct | 09-11-2009
http://www.aavso.org/publications/alerts/alert412.shtml

 

 

Type He/N Nova

Broad lines > 2500 km.s-1
N and He lines

Fast spectral evolution

 

 

 

 

KT Eri | 27-11-2009

 

 

Supernovae

Type SN I
no H lines
deep absorption(SiII) at 6150 angtröms

 

 

 

 

 

 

SN 2011by in NGC3972 |12-05-5011
Type Ia

 

Type SN II
H lines present

 

 

 

 

 

 

 

SN2011dh in M51 | 16-06-2011
Type IIb

     

 

 

 

Comparison between Type I and II supernovae

 

Supernovae lines identification  

 

 

Classification of supernovae
Turatto, 2003 : http://arxiv.org/abs/astro-ph/0301107

http://ned.ipac.caltech.edu/level5/March03/Filippenko/frames.html

http://supernova.lbl.gov/~dnkasen/tutorial/

http://www.uni.edu/morgans/astro/course/Notes/section2/new9.html

http://www.astro.rug.nl/~onderwys/ACTUEELONDERZOEK/JAAR2001/rico/spectra.html

http://www.cfa.harvard.edu/supernova/RecentSN.html

http://marwww.in2p3.fr/~blondin/graphics/index.html

http://supernova.lbl.gov/~nugent/nugent_templates.html

 

 

On novae spectral evolution : http://www.astronomie-amateur.fr/Projets%20Spectro4%20Novae.html (in french)

Further readings, with many spectra :

The formation of novae spectra
R.E. Williams
A.J., Vol. 104, Number 2, 1992

The evolution and classification of postoutburst novae spectra
R.E. Williams & al.
A.J., 376:721-737, 1991

The Tololo nova survey : spectra of recent novae
R.E. Williams, M.M. Phillips, M. Hamuy
A.J. supp. ser., 90:297-316, 1994

 

 

 

 

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