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相关论文: Giant Lyman-Alpha Nebulae in the Illustris Simulat…

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The recent discovery by Cantalupo et al. (2014) of the largest (~500 kpc) and luminous Ly-alpha nebula associated with the quasar UM287 (z=2.279) poses a great challenge to our current understanding of the astrophysics of the halos hosting…

星系天体物理 · 物理学 2015-09-09 Fabrizio Arrigoni Battaia , Joseph F. Hennawi , J. Xavier Prochaska , Sebastiano Cantalupo

Several decades of observations and discoveries have shown that high-redshift AGN and massive galaxies are often surrounded by giant Lyman-alpha nebulae extending in some cases up to 500 kpc in size. In this review, I discuss the properties…

星系天体物理 · 物理学 2017-05-31 Sebastiano Cantalupo

Circumgalactic Lyman-alpha (Ly$\alpha$) nebulae are gaseous halos around galaxies exhibiting luminous extended Ly$\alpha$ emission. This work investigates Ly$\alpha$ nebulae from deep imaging of $\sim12~\mathrm{deg}^2$ sky, targeted by the…

Recent theoretical work has suggested that Lyman-alpha nebulae could be substantially polarized in the Lyman-alpha emission line, depending on the geometry, kinematics, and powering mechanism at work. Polarization observations can therefore…

宇宙学与河外天体物理 · 物理学 2015-05-27 Moire K. M. Prescott , Paul S. Smith , Gary D. Schmidt , Arjun Dey

Direct Ly $\alpha$ imaging of intergalactic gas at $z\sim2$ has recently revealed giant cosmological structures around quasars, e.g. the Slug Nebula (Cantalupo et al. 2014). Despite their high luminosity, the detection rate of such systems…

In an effort to search for Ly$\alpha$ emission from circum- and intergalactic gas on scales of hundreds of kpc around $z\sim3$ quasars, and thus characterise the physical properties of the gas in emission, we have initiated an extensive…

The Nilsson et al. (2006) Lyman-alpha nebula has often been cited as the most plausible example of a Lyman-alpha nebula powered by gravitational cooling. In this paper, we bring together new data from the Hubble Space Telescope and the…

星系天体物理 · 物理学 2015-06-23 Moire K. M. Prescott , Ivelina Momcheva , Gabriel B. Brammer , Johan P. U. Fynbo , Palle Møller

The Slug Nebula is one of the largest and most luminous Lyman-alpha (LyA) nebulae discovered to date, extending over 450 kiloparsecs (kpc) around the bright quasar UM287 at z=2.283. Characterized by high surface brightnesses over…

星系天体物理 · 物理学 2018-07-25 Camille N. Leibler , Sebastiano Cantalupo , Bradford P. Holden , Piero Madau

The recent discovery of enormous Ly$\alpha$ nebulae (ELANe), characterized by physical extents $>200$ kpc and Ly$\alpha$ luminosities $>10^{44}$ erg s$^{-1}$, provide a unique opportunity to study the intergalactic and circumgalactic medium…

The CGM around unobscured AGN has received much attention in recent years. Comparatively, nebulae associated with obscured AGN are less studied. Here, we simulate the Ly$\alpha$, H$\alpha$, and HeII nebulae around the two types of AGN at…

We performed long-slit optical spectroscopy (GTC-OSIRIS) of 6 radio-loud QSOs at redshifts $2<z<3$, known to have giant ($\sim 50$-100 kpc) Lyman-$\alpha$ emitting nebulae, and detect extended Lyman-$\alpha$ emission for 4, with surface…

星系天体物理 · 物理学 2015-06-22 Nathan Roche , Andrew Humphrey , Luc Binette

In the context of the FLASHLIGHT survey, we obtained deep narrow band images of 15 $z\sim2$ quasars with GMOS on Gemini-South in an effort to measure Ly$\alpha$ emission from circum- and inter-galactic gas on scales of hundreds of kpc from…

宇宙学与河外天体物理 · 物理学 2016-10-19 Fabrizio Arrigoni Battaia , Joseph F. Hennawi , Sebastiano Cantalupo , J. Xavier Prochaska

It has been well established in the local universe that galaxy properties differ based on the large-scale environment in which they reside. As luminous Lyman-alpha nebulae have been shown to trace overdense environments at z~2-3, comparing…

星系天体物理 · 物理学 2023-01-11 Natalie K. Wells , Moire K. M. Prescott , Kristian M. Finlator

"Ly$\alpha$ nebulae" are giant ($\sim$100 kpc), glowing gas clouds in the distant universe. The origin of their extended Ly$\alpha$ emission remains a mystery. Some models posit that Ly$\alpha$ emission is produced when the cloud is…

星系天体物理 · 物理学 2020-05-13 Eunchong Kim , Yujin Yang , Ann Zabludoff , Paul Smith , Buell Jannuzi , Myung Gyoon Lee , Narae Hwang , Byeong-Gon Park

We present a study of an extended Lyman-alpha (Lya) nebula located in a known overdensity at z~2.38. The data include multiwavelength photometry covering the rest-frame spectral range from 0.1 to 250um, and deep optical spectra of the…

宇宙学与河外天体物理 · 物理学 2014-11-20 C. Scarlata , J. Colbert , H. I. Teplitz , C. Bridge , P. Francis , P. Palunas , B. Siana , G. M. Williger , B. Woodgate

We examine the cooling radiation from forming galaxies in hydrodynamic simulations of the LCDM model (cold dark matter with a cosmological constant), focusing on the Ly-alpha line luminosities of high-redshift systems. Primordial…

天体物理学 · 物理学 2010-11-04 Mark A. Fardal , Neal Katz , Jeffrey P. Gardner , Lars Hernquist , David H. Weinberg , Romeel Davé

[abbreviated] We present a census of Ly\alpha\ emission at $z\gtrsim7$ utilizing deep near infrared HST grism spectroscopy from the first six completed clusters of the Grism Lens-Amplified Survey from Space (GLASS). In 24/159…

Large nebulae (>50 kpc) emitting strongly in Lya (also known as Lya ``blobs'') are likely signposts of ongoing massive galaxy formation. The relative rarity of these sources and their discovery in well-studied galaxy overdensities suggest…

天体物理学 · 物理学 2009-11-13 M. K. M. Prescott , N. Kashikawa , A. Dey , Y. Matsuda

We present the discovery of a giant $\gtrsim$100~kpc Ly$\alpha$ nebula detected in the core of the X-ray emitting cluster CL~J1449+0856 at $z=1.99$ through Keck/LRIS narrow-band imaging. This detection extends the known relation between…

We present results of a survey for giant Ly-alpha nebulae (LABs) at z=3 with Subaru/Suprime-Cam. We obtained Ly-alpha imaging at z=3.09+-0.03 around the SSA22 protocluster and in several blank fields. The total survey area is 2.1 square…

宇宙学与河外天体物理 · 物理学 2015-05-20 Y. Matsuda , T. Yamada , T. Hayashino , R. Yamauchi , Y. Nakamura , N. Morimoto , M. Ouchi , Y. Ono , K. Kousai , E. Nakamura , M. Horie , T. Fujii , M. Umemura , M. Mori
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