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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.

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

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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