Calendar

Nov
6
gio
Lezione Corso: “Magnetohydrodynamics in Astrophysical Processes”
Nov 6@9:00–12:00
Seminario: Maria Messineo (UniBo)
Nov 6@15:00–17:00

Titolo: Bright late-type stars in the thin Disk of the Milky Way

 

Abstract: Red supergiants (RSGs) and asymptotic giant branch (AGB) stars are the
brightest sources at infrared wavelengths, detectable at a distance
of a few  megaparsecs —- even in heavily obscured galactic centers.
Through winds and mass loss, they enrich and sculpt the interstellar
medium.
Despite similar spectral energy distributions and apparent magnitudes,
RSGs and AGBs trace distinct spatial structures of a galaxy.
AGBs trace well the gravitational potential, including the central bar,
and span ages from 50 Myr to a Hubble time. RSGs, aged 4.5–40 Myr, decorate
the spiral arms, the central molecular disk, and the bar’s endpoints.
The Milky Way offers the nearest laboratory for resolved stellar
populations
in a barred galaxy, however, dust obscuration and distance uncertainties
hinder
clean separation of RSGs and AGBs -— a critical step for mapping Disk
structure
and star-formation history.
Over the past several years, I have developed methods to estimate
extinction
by partitioning interstellar and circumstellar components, to obtain better
luminosity and to distinguish RSGs from AGBs. I will highlight key
challenges
and solutions, including extinction-free colors as interstellar
extinction proxies,
GLIMPSE color–color diagrams, and Gaia–2MASS criteria.
Finally, I will present a new Gaia catalog of ~700 bona fide optical RSGs,
detailing its construction, temperature, and luminosity characterization.

Nov
11
mar
Seminario: Elina Lindfors (University of Turku)
Nov 11@10:00–12:00

Titolo: Association of the astrophysical neutrinos with flares from relativistic jets launched by supermassive black holes?

 

Abstract:

Over the past decade, the IceCube Neutrino Observatory has detected a few hundreds of high-energy (HE) neutrinos from cosmic sources. Despite numerous studies searching for their origin, it is still not known which source populations emit them. A few confident individual associations exist with active galactic nuclei (AGN), mostly with blazars which are jetted AGN whose jet points in our direction. Nonetheless, on a population level, blazar-neutrino correlation strengths are rather weak. To definitively answer if jetted AGN systematically emit >~100 TeV neutrinos: (1) we compiled the largest catalog of blazars and their optical light curves to date; and (2) we searched for a spatio-temporal correlation between these blazar light curves and IceCube’s first catalog of >~100 TeV neutrino events while assuming that neutrinos are expected at the brightest optical outbursts. Under this phenomenological assumption, we found that a global blazar-neutrino correlation cannot be confidently established, inline with the result of our previous study in the radio band. We estimated that fewer than ~8% of >~100TeV neutrino events came from major blazar outbursts, alluding to substantial contributions from other systems. In my talk, I will present this state-of-the-art correlation study and outlook for further searches with next generation of instruments.
Nov
13
gio
Seminario: Maria Luisa Tuscano (INAF-OAPa)
Nov 13@15:30–17:30

Title: Piazzi e la Meridiana della Cattedrale di Palermo

Abstract: La realizzazione della meridiana a camera oscura nella Cattedrale di Palermo costituisce una
testimonianza dell’impegno assunto da Giuseppe Piazzi non solo nel quadro di potenziamento dello
studio dell’Astronomia, ma anche verso iniziative sociali volte al benessere del territorio e
all’affermazione di Palermo nel contesto internazionale.
Gli anni trascorsi a Londra avevano fatto apprezzare all’astronomo l’adozione del Tempo medio
nell’ambito dello sviluppo economico legato alla prima rivoluzione industriale.
La riforma della misura del Tempo nella città di Palermo costituì per Piazzi un obiettivo sociale da
raggiungere attraverso un graduale processo educativo del territorio, in cui era ancora in uso l’orario
italico civile.
La meridiana, misurando il tempo astronomico, costituiva l’anello di congiunzione per la successiva
introduzione del tempo medio
Ma l’individuazione di Cerere limitò in parte il piano di Piazzi che, comunque ci lascia uno strumento
molto apprezzato a livello mondiale e di cui si auspica un’adeguata preservazione per il suo peculiare
valore scientifico e didattico.

Nov
18
mar
Lezione Corso: “Magnetohydrodynamics in Astrophysical Processes”
Nov 18@9:00–12:00
Nov
20
gio
Lezione Corso: “Magnetohydrodynamics in Astrophysical Processes”
Nov 20@9:00–12:00
Nov
21
ven
Lezione Corso: “Magnetohydrodynamics in Astrophysical Processes”
Nov 21@9:00–12:00
Nov
25
mar
PROVA ORALE CONCORSO CTER T.I
Nov 25 giorno intero
Dic
12
ven
Presentazione Risultati ExoSchool II
Dic 12@9:00–18:00
Dic
18
gio
Seminario: Alberto Traina (INAF-OAS Bologna) @ Aula
Dic 18@15:00–16:30
Speaker: Alberto Traina (INAF-OAS Bologna)
Title: SMBHs growth in overdense environments: AGN enhancement in protoclusters with enormous Ly⍺ nebulae
Abstract: SMBHs are almost ubiquitous in galaxies’ nuclei in the local and in the high-redshift Universe. However, the formation and growth processes that lead to such massive objects in relatively short timescales are still unclear. A crucial role in accelerating their evolution may be played by the surrounding environment: large quantities of gas and higher merger rates are key to understand how their growth occurs. Protoclusters of galaxies, the precursors of today’s galaxy clusters, represent the perfect laboratories to investigate this effect at high redshift. The hunt for the SMBHs population in protoclusters and its characterization requires a multi-wavelength effort to obtain a complete census: in this perspective the X-rays represent the best channel to investigate the AGN activity, even in the most obscured conditions. In this talk, I will present recent deep (>200ks) Chandra observations targeting three protoclusters at z ~ 2-3, that host enormous Ly⍺ nebulae. I will discuss the spectral properties of the detected AGN as well as the effects of overdense environment on the growth of SMBHs. In particular, I will show the fraction of AGN and the X-ray luminosity functions of the protoclusters, which are significantly larger (1 – 2 dex!) than those of their local counterparts. I will present new results on how the enhancement of SMBHs in overdense environments (x10 larger than SMGs) suggests that protoclusters are indeed optimal sites for promoting their growth. Finally, I will show preliminary results on the growth of SMBHs in hydrodynamical cosmological simulations.