Scheda JaDO FINAL




Informazioni generali

Jets and Dusty Outflows in young stars

JaDO

Progetto

Programma

Infrastruttura Internazionale

RSN2

Attività: In Itinere; Data inizio: 2023; Data fine: 2025

elisabetta.rigliaco elisabetta.rigliaco@inaf.it


Il programma JaDO e' volto a studiare la presenza di getti e Outflows polverosi intorno a stelle giovani. Data la loro natura polverosa questi getti ed outflows sono rilevabili principalmente con tecniche di immagini ad alto contrasto, in particolare in polarimetria, come per esempio quello fornito da SPHERE/VLT. 

Lo scopo del programma e' quello di studiare le caratteristiche di getti e outflows polverosi in un campione di stelle osservate con SPHERE/VLT come parte di GTO e Large Programs, come e’ stato gia’ fatto per alcune stelle come RCrA e TCrA. 

The JaDO program aims at the analysis of Jets and Dusty Outflows around young stars. These kind of jets and outflows are better seen using high contrast imaging techniques, such as polarimetric observations. These kind of observations are provided for example by SPHERE/VLT. The program aims at the analysis of the characteristics of Jets and Dusty outflows in a sample of young stars already observed with SPHERE/VLT as part of GTO and Large programs. These kind of studies have been already performed in sources as RCrA and TCrA.  

Mezzo interstellare, formazione di stelle e sistemi planetari


Team Summary

15. Personale INAF coinvolto
Numero di partecipanti INAF al progetto: 1
Struttura Nfte N0 TI 2023 TI 2024 TI 2025 TD 2023 TD 2024 TD 2025 Nex Extra
O.A. PADOVA 1 0 0.30 0.30 0.00 0 0 0 0 0.00
Totali 1 0 0.30 0.30 0.00 0.00 0.00 0.00 0 0.00

Fondi a sostegno

21. Totale fondi a disposizione (dato aggregato, k€)
Certi 2023 Certi 2024 Certi 2025 Presunti 2023 Presunti 2024 Presunti 2025
5000.0 10000.0 5000.0 0.0 0.0 0.0

Produzione scientifica e tecnologica

22. Produzione scientifica e tecnologica - Highlights
# DOI Descrizione Azione
1 10.48550/arXiv.2301.01486 Titolo: Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS)Autori: E. Rigliaco and R. Gratton and ... Published: EPD Sciences Rivista: Astronomy\&amp$\mathsemicolon$ Astrophysics Anno pubblicazione: 2023
2 10.1051/0004-6361/201936707 Titolo: Investigating the nature of the extended structure around the Herbig star RCrA using integral field and high-resolution spectroscopy Autori:E. Rigliaco and R. Gratton and D. Mesa and V. D'Orazi and M. Bonnefoy and J. M. Alcal\`a and S. .... Publisher:EDP Sciences Rivista: Astronomy \&amp$\mathsemicolon$ Astrophysics Anno pubblicazione:2019



Informazioni Pubbliche

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left: 35.040000915527344%; top: 41.150001525878906%; font-family: sans-serif;">r</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 35.4900016784668%; top: 41.150001525878906%; font-family: sans-serif;">&nbsp;</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 35.869998931884766%; top: 41.150001525878906%; font-family: sans-serif;">o</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 36.65999984741211%; top: 41.150001525878906%; font-family: sans-serif;">b</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 37.470001220703125%; top: 41.150001525878906%; font-family: sans-serif;">j</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 37.77000045776367%; top: 41.150001525878906%; font-family: sans-serif;">e</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 38.5%; top: 41.150001525878906%; font-family: sans-serif;">c</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 39.2400016784668%; top: 41.150001525878906%; font-family: sans-serif;">t</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 39.66999816894531%; top: 41.150001525878906%; font-family: sans-serif;">s</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 40.349998474121094%; top: 41.150001525878906%; font-family: sans-serif;">&nbsp;</span></div>

<p><font face="sans-serif">The PI of this scheda is part of the large program JEDI (PI: Nisini). Moreover she plays also&nbsp;</font><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 70.83000183105469%; top: 62.54999923706055%; font-family: sans-serif;">responsibilities roles in&nbsp;</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 34.650001525878906%; top: 62.54999923706055%; font-family: sans-serif;">international p</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 35.459999084472656%; top: 62.54999923706055%; font-family: sans-serif;">r</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 35.88999938964844%; top: 62.54999923706055%; font-family: sans-serif;">o</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 36.68000030517578%; top: 62.54999923706055%; font-family: sans-serif;">j</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 36.97999954223633%; top: 62.54999923706055%; font-family: sans-serif;">e</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 37.720001220703125%; top: 62.54999923706055%; font-family: sans-serif;">c</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 38.45000076293945%; top: 62.54999923706055%; font-family: sans-serif;">t</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 38.880001068115234%; top: 62.54999923706055%; font-family: sans-serif;">s</span><span role="presentation" dir="ltr" style="font-size: calc(var(--scale-factor)*8.01px); left: 70.83000183105469%; top: 62.54999923706055%; font-family: sans-serif;">&nbsp;such as the&nbsp;</span><span style="font-size: 11pt; font-family: Arial; color: rgb(0, 0, 0); font-variant-ligatures: normal; font-variant-east-asian: normal; font-variant-position: normal; vertical-align: baseline; white-space: pre-wrap;"> SPHERE-DESTINYS Large Programme </span></p>

<p>INAF; UCL (Department of Space and Climate Physics); University of Galway</p>


15. Team members, Informazioni generali


15. Personale INAF coinvolto

# Nome E-mail Struttura TI Qualifica Ruolo nel Progetto FTE Impegnate (2023/2024/2025) FTE Presunte (2023/2024/2025) Extra
1 elisabetta.rigliaco elisabetta.rigliaco@inaf.it O.A. PADOVA Y RICERCATORE coordinatore X X X X X X X OK

16. Personale Associato INAF coinvolto

# Nome E-mail Struttura TI Qualifica Ruolo nel Progetto FTE Impegnate (2023/2024/2025) FTE Presunte (2023/2024/2025) Extra

21. Fondi a Sostegno Iniziativa

This project has been awarded 20K euro in the call of mini-grant 2022.


Tabella fondi:

# Provenienza Certi 2023 (k€) Certi 2024 (k€) Certi 2025 (k€) Presun. 2023 (k€) Presun. 2024 (k€) Presun. 2025 (k€) Totale Certi (k€) Totale Presunti (k€)
1 Mini-Grant 2022 5000 10000 5000 0 0 0 20000 0


Tabella fondi Astrofisica Fondamentale e PNRR:
# Provenienza Fondi 2023 (€) Fondi 2024 (€) Fondi 2025 (€)