Very good result.
Page in the database: https://aras-database.github.io/databas ... 2024b.html
François
Search found 1561 matches
- Fri Apr 05, 2024 1:53 pm
- Forum: Miscellanous
- Topic: AT 2024fjh -another LMC nova?
- Replies: 4
- Views: 224
- Sun Mar 24, 2024 10:01 am
- Forum: Miscellanous
- Topic: AT2024epj - A mag 10 transient in/near the LMC
- Replies: 12
- Views: 2442
Re: AT2024epj - A mag 10 transient in/near the LMC
Great observations.
Congratulations
The emergence of He II 4686 on the red edge of the complex NIII/CIII
François
Congratulations
The emergence of He II 4686 on the red edge of the complex NIII/CIII
François
- Wed Mar 20, 2024 5:01 pm
- Forum: Miscellanous
- Topic: AT2024epj - A mag 10 transient in/near the LMC
- Replies: 12
- Views: 2442
Re: AT2024epj - A mag 10 transient in/near the LMC
Good result despite the low luminosity
Very fast nova.
Expansion velocity 4900-5100 km/s measured on H alpha and H beta.
Page opened: https://aras-database.github.io/database/at2024epj.html
Very fast nova.
Expansion velocity 4900-5100 km/s measured on H alpha and H beta.
Page opened: https://aras-database.github.io/database/at2024epj.html
- Wed Mar 13, 2024 10:28 am
- Forum: Novae
- Topic: Nova Oph 2024
- Replies: 1
- Views: 585
Re: Nova Oph 2024
Impressive! Very high velocity.
Thus nova event produced by a high mass white dwarf, small mass of the accreted envelop and large part of the envelop ejected.
Congratulations.
Page opened: https://aras-database.github.io/databas ... h2024.html
Thus nova event produced by a high mass white dwarf, small mass of the accreted envelop and large part of the envelop ejected.
Congratulations.
Page opened: https://aras-database.github.io/databas ... h2024.html
- Thu Mar 07, 2024 6:30 pm
- Forum: Introduction / Présentation
- Topic: Présentation Pierre-Bernard Toubol
- Replies: 2
- Views: 1746
Re: Présentation Pierre-Bernard Toubol
Bonjour Pierre-Bernard,
Une démarche trés intéressante.
Peux-tu nous montrer un example ou deux?
Bienvenue sur le Forum
François Teyssier
Une démarche trés intéressante.
Peux-tu nous montrer un example ou deux?
Bienvenue sur le Forum
François Teyssier
- Wed Mar 06, 2024 8:38 am
- Forum: Astrophysics, Theory, Publications ...
- Topic: Conference Small Telescopes 2023 Proceedings
- Replies: 0
- Views: 2203
Conference Small Telescopes 2023 Proceedings
PROCEEDINGS OF THE WORKSHOP OBSERVING TECHNIQUES, INSTRUMENTATION AND SCIENCE FOR METRE-CLASS TELESCOPES III September 11 – 15, 2023, Tatranská Lomnica, Slovaki https://www.ta3.sk/caosp/Eedition/Abstracts/2024/Vol_54/No_2/ Full text: https://www.ta3.sk/caosp/Eedition/FullTexts/vol54no2/caosp54_2.pdf...
- Tue Feb 13, 2024 8:17 am
- Forum: Novae
- Topic: PNV J17261813-3809354
- Replies: 15
- Views: 1261
Re: PNV J17261813-3809354
Excellent!
Page open in the database: https://aras-database.github.io/databas ... o2024.html
Bonne continuation!
François
Page open in the database: https://aras-database.github.io/databas ... o2024.html
Bonne continuation!
François
- Tue Feb 06, 2024 9:48 am
- Forum: Introduction / Présentation
- Topic: Présentation de Olivier Cheurfi
- Replies: 1
- Views: 5521
Re: Présentation de Olivier Cheurfi
Bienvenue Olivier.
A voir les spectres de bet et eps Ori que tu présentes, les débuts sont plutôt bien maîtrisés! Excellent.
A voir les spectres de bet et eps Ori que tu présentes, les débuts sont plutôt bien maîtrisés! Excellent.
- Tue Feb 06, 2024 9:46 am
- Forum: Astrophysics, Theory, Publications ...
- Topic: Publications using ARAS ES spectra in 2023
- Replies: 0
- Views: 851
Publications using ARAS ES spectra in 2023
Here's a list of papers using ARAS Eruptive Stars database in 2023. 1 Revisiting the classics: on the evolutionary origin of the 'Fe II' and 'He/N' spectral classes of novae Aydi, E., Chomiuk, L., Strader, J., Sokolovsky, K. V., Williams, R. E., Buckley, D. A. H., & al. (18) Monthly Notices of t...
- Tue Feb 06, 2024 9:35 am
- Forum: Symbiotic Stars
- Topic: T CrB before its new nova event
- Replies: 27
- Views: 15857
Re: T CrB before its new nova event
The new season of observations after the solar conjunction is begining. Since the detection of the end of the high state (2015-2023), T CrB evolves in the same way as before the high state with orbital variations of the photometry and spectroscopic appearence. TCrB_1dayMean_cleaned.png First spectra...