V335 Vul

Information about outbursts of eruptive stars, Be activity, ...
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Francois Teyssier
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V335 Vul

Post by Francois Teyssier »

Poalo Berardi has obtained a spectrum of V335 Vul at medium resolution (R = 5000)
V335Vul.PNG
V335Vul.PNG (21.13 KiB) Viewed 7258 times
V335 is suspected symbiotic in Belczinski & al. catalog
The Ha line is very narrow for a symbiotic (67 km/s in Paolo's spectrum)
The red giant is a carbon star
Mag ~ 11.8

A low resolution spectrum should be welcome in the next Information letter



François
Joan Guarro Flo
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Joined: Thu Nov 03, 2011 8:50 pm

Re: V335 Vul

Post by Joan Guarro Flo »

To all :

This graph of V335 Vul, complemented the observation of Paolo.

Regards, Joan.
Attachments
_v335vul_20160822_881_J. Guarro.png
_v335vul_20160822_881_J. Guarro.png (7.11 KiB) Viewed 7218 times
Francisco Campos
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Re: V335 Vul

Post by Francisco Campos »

Hello,

here is my contribution, taken the last night.

Joan, you observed at the same time as me. Quina casualitat! :mrgreen:
_v335vul_20160822_851.png
_v335vul_20160822_851.png (9.28 KiB) Viewed 7207 times
Greetings
Fran
Francois Teyssier
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Re: V335 Vul

Post by Francois Teyssier »

Thank you Joan and Fran
It will be interesting to compare the instrumental response

Comments of Belczinski & al. in their Catalog of Symbiotics :
V335 Vul Suspected in [225]: presence of carbon giant and optical emission-line spectrum (H i) displaying hot continuum in blue. We agree with this classification although this object might be a single pulsating star: (i) the carbon star might pulsate with period of 342 days [55]and then emission lines behave as for a Mira variable – they disappear near minimum light and show up again at maximum (see spectra in [225]); (ii) Hα is very narrow:
2˚A (90 km s−1) and for a symbiotic star we would expect a width of about 300–500 km s−1; (iii) the Balmer decrement is different than that observed for symbiotic stars (it resembles that of Mira variable), although the authors of [225] claim that the Balmer decrement resembles that of a symbiotic star.

[225} = Munari, U., Tomov, T., Rejkuba, M., 1998, Inf. Bull. Variable Stars 4668
See also : Dahlmark, L., 1994, J. Am. Assoc. Variable Star Obs. 23, 34 for the period

François
Francois Teyssier
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Re: V335 Vul

Post by Francois Teyssier »

Pas mal !
V335Vul.PNG
V335Vul.PNG (16.82 KiB) Viewed 7197 times
Bonne continuation,

François
Joan Guarro Flo
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Re: V335 Vul

Post by Joan Guarro Flo »

CONGRATULATIONS, Fran !!

(Una mica més i ens cau el pèl ), Joan.
Olivier Thizy
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Re: V335 Vul

Post by Olivier Thizy »

Hello,,


to have some fun and push my equipment I did 4h15min on V335 Vul tonight. Not all individual spectra are ok but the outcome is still nice with lot of details and an overall shape which looks like the one published here before.

Here is:
-the spectrum from 5000A (below it is very noisy, maybe I should I go to Hbeta...
-a zoom on Halpha and above, this start beeing very red.
-the astrometry on my guiding image
-the overall screen of the PC observatory during the acquisitions...
graph_v335vul_20160823_854_full-all.png
graph_v335vul_20160823_854_full_zoom.png
Capture V335 Vul astrometry ok.JPG
Capture V335 Vul astrometry ok.JPG (83.9 KiB) Viewed 7176 times
Capture V335Vul2.JPG


Cordialement,
Olivier Thizy
Joan Guarro Flo
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Re: V335 Vul

Post by Joan Guarro Flo »

Il est un bon document, Olivier !
Tu sais, ce observer la V335 Vul est pas facile.
Joan.
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