Symbiotic recurrent nova RS Oph in ourburst !!!
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
hello,
comparison of low-res spectra of RS Oph from 09 to 14th Aug:
vincent
comparison of low-res spectra of RS Oph from 09 to 14th Aug:
vincent
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
...and including this night :
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
Observation of RS Oph by using a 65 mm refractor (2.5-inch) and Star'Ex at nearly maximal resolution of the setup; i.e. R=30 000 (for 8 x 600 sec. exposure):
Detail of H-alpha peak (fading); well resolved and after H2O lines removal:
Christian Buil
Detail of H-alpha peak (fading); well resolved and after H2O lines removal:
Christian Buil
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
Here is my LhiresIII shot of RS Oph on 15Aug21:
The H-Alpha spike seems to be getting shorter with the "fan" below getting wider.
James
The H-Alpha spike seems to be getting shorter with the "fan" below getting wider.
James
James Foster
eShel2-Zwo ASI6200MM Pro
Lhires III (2400/1800/600 ln/mm Grat) Spectroscope
LISA IR/Visual Spectroscope (IR Configured)
Alpy 200/600 with Guide/Calibration modules and Photometric slit
Star Analyzer 200
eShel2-Zwo ASI6200MM Pro
Lhires III (2400/1800/600 ln/mm Grat) Spectroscope
LISA IR/Visual Spectroscope (IR Configured)
Alpy 200/600 with Guide/Calibration modules and Photometric slit
Star Analyzer 200
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
Bonsoir
Nova proche l'UV ce soir
reseau pas optimal !
UVEX(4), G600 750nm, RC8, slit 23µ
La Lune commence à gêner un peu !
Pierre
Nova proche l'UV ce soir
reseau pas optimal !
UVEX(4), G600 750nm, RC8, slit 23µ
La Lune commence à gêner un peu !
Pierre
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
finally joining the party after some equipment drownings last week. 10 minutes at low altitude (21 degrees) with 175mm newtonian at f7, and an L200 littrow, 180lpmm grating.
No sign of pi cyg profiles any more in my spectrum.
Is anyone managing a central location for uploading fits files of spectra of this object?
I see Christian is pushing the limits with star'ex, amazing work!
No sign of pi cyg profiles any more in my spectrum.
Is anyone managing a central location for uploading fits files of spectra of this object?
I see Christian is pushing the limits with star'ex, amazing work!
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
The ARAS, BAA and AAVSO databases are all accepting spectra of RS OphHamish Barker wrote:
Is anyone managing a central location for uploading fits files of spectra of this object?
In ARAS you can find it under the Symbiotics here
https://aras-database.github.io/database/rsoph.html
Cheers
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
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
Hello Hamisch
You can not detect Ca V or Fe VI at this state.
High ionized lines will appear later when the envelop (and photo-sphere) will recede sufficiently and their temperature increase to about ~100 kK and more.
At the current state, the temperature is about 30 kK ([OIII] for example is raising).
François
You can not detect Ca V or Fe VI at this state.
High ionized lines will appear later when the envelop (and photo-sphere) will recede sufficiently and their temperature increase to about ~100 kK and more.
At the current state, the temperature is about 30 kK ([OIII] for example is raising).
François
François Teyssier
http://www.astronomie-amateur.fr
http://www.astronomie-amateur.fr
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
Thank you Francois,
I thought that those IV and V lines were likely not the correct ones, but couldn't see other likely ones in the short list which I had on hand. what do you think they are likely to be?
I thought that those IV and V lines were likely not the correct ones, but couldn't see other likely ones in the short list which I had on hand. what do you think they are likely to be?
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Re: Symbiotic recurrent nova RS Oph in ourburst !!!
Hello all,
Not so easy to follow the RS Oph outburst with the parade of clouds the last few days !!
Here is a comparison between my three last spectra the Halpha line of RS Oph at high resolution on August 12 at 21 h 24 TU (resolution of 16932, JJ = 2459439.3915, acquisition time of 70 min (7 x 600s)), on August 19 at 22 h 19 TU (resolution of 18039, JJ = 2459446.4296, acquisition time of 10 min (1 x 600s)) and on August 20 at 21 h 12 TU (resolution of 18575, JJ = 2459447.3835, acquisition time of 50 min (5 x 600s)) obtained with my LHIRES III (grating of 2400 lines / mm) and the previous one, on August 11.
What a dramatic change in the profile of the Halpha line in a few days !!
Clear skies to all !!
Christophe BOUSSIN
Not so easy to follow the RS Oph outburst with the parade of clouds the last few days !!
Here is a comparison between my three last spectra the Halpha line of RS Oph at high resolution on August 12 at 21 h 24 TU (resolution of 16932, JJ = 2459439.3915, acquisition time of 70 min (7 x 600s)), on August 19 at 22 h 19 TU (resolution of 18039, JJ = 2459446.4296, acquisition time of 10 min (1 x 600s)) and on August 20 at 21 h 12 TU (resolution of 18575, JJ = 2459447.3835, acquisition time of 50 min (5 x 600s)) obtained with my LHIRES III (grating of 2400 lines / mm) and the previous one, on August 11.
What a dramatic change in the profile of the Halpha line in a few days !!
Clear skies to all !!
Christophe BOUSSIN
CBO (Newton 200 F/5 / Alpy600 / Atik 314L+ / Atik Titan + Mewlon 180 F/12 / LHIRES III 2400 / Atik 460EX / Atik 314 L+) @ ARAS database