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Hot Milk SIGNED

Flows of hot plasma connecting the Milky Way centre to the corona, halo and beyond

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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 Hot Milk project word cloud

Explore the words cloud of the Hot Milk project. It provides you a very rough idea of what is the project "Hot Milk" about.

containing    away    interplay    telescopes    plasma    depends    emitting    view    parsec    connection    instruments    spiral    outflows    gc    invaluable    erc    re    orders    local    erosita    prototype    array    agn    feedback    galaxy    medium    plane    energetic    missing    rectify    03    band    unknown    fundamental    obscuration    hot    coverage    wavelength    kpc    beginning    limited    improvement    interstellar    soft    opportunity    energy    additionally    galaxies    stellar    existence    disc    sub    capture    cosmic    feasibility    neighbourhood    rosat    harder    offers    halo       ingredient    galactic    phases    imaging    solar    evolution    sensitive    critically    horizon    milky    candidate    centre    baryons    maps    affairs    outside    confirmed    revolution    universe    basically    approved    magnitude    sky    xmm    despite    surveys    condensation    covered    generation    narrow    sensitivity    scales    ray    survey    rays    trace    legacy    corona    details    plausible    confirming    traced    ism   

Project "Hot Milk" data sheet

The following table provides information about the project.

Coordinator
ISTITUTO NAZIONALE DI ASTROFISICA 

Organization address
address: VIALE DEL PARCO MELLINI 84
city: ROMA
postcode: 136
website: www.inaf.it

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Italy [IT]
 Total cost 1˙989˙375 €
 EC max contribution 1˙989˙375 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2019-COG
 Funding Scheme ERC-COG
 Starting year 2020
 Duration (year-month-day) from 2020-03-01   to  2025-02-28

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    ISTITUTO NAZIONALE DI ASTROFISICA IT (ROMA) coordinator 1˙264˙375.00
2    MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV DE (MUENCHEN) participant 725˙000.00

Map

 Project objective

We are less than one year away from the beginning of a revolution in our understanding of the hot, X-ray emitting, plasma of the Milky Way. The growth of galaxies in the local Universe critically depends on the interplay (via outflows and re-condensation) between the hot plasma with the other phases of the interstellar medium (ISM). As a prototype for typical spiral galaxies, the Milky Way offers the unique opportunity to capture the important details of such feedback all the way from sub-parsec to galactic scales. In the 90's, the ROSAT all-sky X-ray maps confirmed the existence of a hot component of the ISM, the Galactic corona. However, because of strong obscuration in the soft X-ray energy band, those maps have a limited horizon of ~1 kpc in the Galactic plane. Therefore, despite the fundamental role of the hot ISM phase, its properties are still basically unknown outside the Solar neighbourhood. My XMM surveys of the Galactic centre (GC) demonstrate that the hot ISM phase can be traced throughout the disc in the harder X-ray band, confirming the feasibility of this ERC project and the strong connection between GC activity and the Galactic corona. Additionally, the hot plasma is a plausible candidate for containing the missing Galactic baryons and a key ingredient for galaxy evolution. However, so far only less than 0.03% of the Milky Way has been covered by the narrow fields of view of current X-ray imaging telescopes. The eROSITA all-sky survey will rectify this state of affairs. Should this ERC proposal be approved, we will trace the connection and feedback between the Galactic corona and halo with the energetic activity at the GC (e.g., due to cosmic rays, stellar and AGN outflows). This will represent one to two orders of magnitude improvement in sensitivity and/or coverage, compared to current surveys. Our sensitive X-ray maps will represent an invaluable legacy for future multi-wavelength studies with current and next generation array instruments.

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The information about "HOT MILK" are provided by the European Opendata Portal: CORDIS opendata.

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lastchecktime (2021-04-22 1:52:22) correctly updated