Type Ia supernovae can be further classified using spectra at maximum light.
The "Branch" classification (Core Normal, Shallow Silicon, Broad Line, Cool) is based on the pseudo equivalent widths of the Si II 5972 and Si II 6355 lines. The pseudo EW and Velocity of the Si II 6355 line can also be used to identify normal and high velocity classes. Based on these systems SN2019ein is Broad Lined, High Velocity and SN2019np is Normal. (See positions overlaid on the graphs from "THE SPECTROSCOPIC DIVERSITY OF TYPE Ia SUPERNOVAE" Blondin et al )
Robin
SN 2019ein
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Re: SN 2019ein
LHIRES III #29 ATIK314 ALPY 600/200 ATIK428 Star Analyser 100/200 C11 EQ6
http://www.threehillsobservatory.co.uk
http://www.threehillsobservatory.co.uk
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Re: SN 2019ein
Hi,
here's my last spectrum of SN2019ein, dated 26th may.
The evolution from 14th may is impressive (spectra corrected from continuum), it's nice to follow such events ! The blue shift has effectively decreased ... . Vincent
here's my last spectrum of SN2019ein, dated 26th may.
The evolution from 14th may is impressive (spectra corrected from continuum), it's nice to follow such events ! The blue shift has effectively decreased ... . Vincent
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Re: SN 2019ein
Summary of your observations gathered in the database: http://www.astrosurf.com/aras/Aras_Data ... 019ein.htm
(Robin Leadbeater, Pascal Le Du, Etienne Bertrand, Christian Buil, Vincent Lecoq, Woody Sims)
Congratulations!
(Robin Leadbeater, Pascal Le Du, Etienne Bertrand, Christian Buil, Vincent Lecoq, Woody Sims)
Congratulations!
François Teyssier
http://www.astronomie-amateur.fr
http://www.astronomie-amateur.fr
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Re: SN 2019ein
Belle observation !
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Re: SN 2019ein
Another spectrum from last night (Taken in twilight. It does not get dark at all here now) The spectrum has evolved more over the last week.
Using SNID, it is a good match to normal type Ia at similar age (~22 days past maximum)
Robin
Using SNID, it is a good match to normal type Ia at similar age (~22 days past maximum)
Robin
LHIRES III #29 ATIK314 ALPY 600/200 ATIK428 Star Analyser 100/200 C11 EQ6
http://www.threehillsobservatory.co.uk
http://www.threehillsobservatory.co.uk