Calendar

dom lun mar mer gio ven sab
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
Il cielo dell’altra metà del cielo: breve storia del contributo delle donne in astronomia seminario di Ileana Chinnici) 15:30
Il cielo dell’altra metà del cielo: breve storia del contributo delle donne in astronomia seminario di Ileana Chinnici) @ Osservatorio Astroomico di Palermo
Feb 15@15:30–17:00
Il talk presenterà alcune figure femminili che hanno contribuito allo sviluppo della scienza astronomica, dalle origini al XX secolo, sottolineando alcuni aspetti che hanno favorito il loro approccio all’astronomia e alcune caratteristiche tipiche del loro contributo. Ileana Chinnici (INAF – Osservatorio Astronomico di Palermo)
16
17
18
19
Properties of solar coronal heating in active regions, from high resolution spectroscopy. Paola Testa (Smithsonian Astrophysical Observatory, USA) 11:00
Properties of solar coronal heating in active regions, from high resolution spectroscopy. Paola Testa (Smithsonian Astrophysical Observatory, USA)
Feb 19@11:00–12:30
Abstract. I will discuss how high spatial, spectral, and temporal resolution chromospheric/transition region/coronal observations coupled with detailed modeling can help us diagnose coronal heating properties in active region cores in non-flaring conditions.  I will focus on recent results from the Interface Region Imaging Spectrograph (IRIS), which provides us with unprecedented high spatial, temporal and spectral resolution observations of the chromosphere
20
21
22
23
24
25
26
TITOLO: A deep X-ray observation of the Class I star Elias 29 with XMM and NuSTAR / Ignazio Pillitteri (INAF-OAPA) 11:30
TITOLO: A deep X-ray observation of the Class I star Elias 29 with XMM and NuSTAR / Ignazio Pillitteri (INAF-OAPA)
Feb 26@11:30–12:30
ABSTRACT: Elias 29 is a Class I star of the young star forming site of the Rho Ophiuchi Dark Cloud.In X-rays it shows a prominent fluorescent line at 6.4 keV which origin is still to be clearly understood. The excitation of fluorescence of cold material could be due to hard X-ray photons especially produced during flares or to high energy
27
28