Search Results - "Afruni, Andrea"

Revealing the Gas Recycling in the Circumgalactic Medium (CGM) Utilizing a Luminous Lya Nebula around a Type II Quasar at z = 2.6 with the Keck Cosmic Web Imager (KCWI) by Zhang, Shiwu, Cai, Zheng, Xu, Dandan, Afruni, Andrea, Wu, Yunjing, Wang, Wuji, Battaia, Fabrizio Arrigoni, Li, Mingyu, Wang, Sen, Bi, Xianzhi

“…Abstract How galaxies acquire material from the circumgalactic medium is a key question in galaxy evolution. Recent observations and simulations show that gas…”
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Most of the cool CGM of star-forming galaxies is not produced by supernova feedback by Afruni, Andrea, Fraternali, Filippo, Pezzulli, Gabriele

“…ABSTRACT The characterization of the large amount of gas residing in the galaxy haloes, the so-called circumgalactic medium (CGM), is crucial to understand…”
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Inflow of low-metallicity cool gas in the halo of the Andromeda galaxy by Afruni, Andrea, Pezzulli, Gabriele, Fraternali, Filippo

“…ABSTRACT As the closest L* galaxy to our own Milky Way, the Andromeda galaxy (M31) is an ideal laboratory for studies of galaxy evolution. The AMIGA project…”
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Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies by Afruni, Andrea, Pezzulli, Gabriele, Fraternali, Filippo, Grønnow, Asger

“…ABSTRACT Galactic halos accrete material from the intergalactic medium (IGM) and part of this accretion is expected to be in the form of cool (T ∼ 104 K) gas…”
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Inflow of low-metallicity cool gas in the halo of the Andromeda galaxy by Afruni, Andrea, Pezzulli, Gabriele, Fraternali, Filippo

“…As the closest $L^{\ast}$ galaxy to our own Milky Way, the Andromeda galaxy (M31) is an ideal laboratory for studies of galaxy evolution. The AMIGA project has…”
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Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies by Afruni, Andrea, Pezzulli, Gabriele, Fraternali, Filippo, Grønnow, Asger

“…Galactic halos accrete material from the intergalactic medium (IGM) and part of this accretion is expected to be in the form of cool ($T\sim10^4$ K) gas. A…”
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Most of the cool CGM of star-forming galaxies is not produced by supernova feedback by Afruni, Andrea, Fraternali, Filippo, Pezzulli, Gabriele

“…The characterization of the large amount of gas residing in the galaxy halos, the so called circumgalactic medium (CGM), is crucial to understand galaxy…”
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Cool circumgalactic gas of passive galaxies from cosmological inflow by Afruni, Andrea, Fraternali, Filippo, Pezzulli, Gabriele

“…A&A 625, A11 (2019) The circumgalactic medium (CGM) of galaxies consists of a multiphase gas with components at very different temperatures, from $10^ {4}$ K…”
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Revealing the Gas Recycling in the Circumgalactic Medium (CGM) Utilizing a Luminous Ly$\alpha$ Nebula Around a Type-II Quasar at z=2.6 with the Keck Cosmic Web Imager (KCWI) by Zhang, Shiwu, Cai, Zheng, Xu, Dandan, Afruni, Andrea, Wu, Yunjing, Wang, Wuji, Battaia, Fabrizio Arrigoni, Li, Mingyu, Wang, Sen, Bi, Xianzhi

“…How galaxies acquire material from the circumgalactic medium (CGM) is a key question in galaxy evolution. Recent observations and simulations show that gas…”
Get full text