Cold streams as Lyman-alpha blobs Collaborators: Avishai Dekel, Amiel Sternberg, Daniel Ceverino, Romain Teyssier, Joel Primack Tobias Goerdt.

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Presentation transcript:

Cold streams as Lyman-alpha blobs Collaborators: Avishai Dekel, Amiel Sternberg, Daniel Ceverino, Romain Teyssier, Joel Primack Tobias Goerdt

Outline Lyman alpha blob observations Cold streams in theory and simulations The AMR simulations Computing the Lyman alpha luminosity Resulting surface brightness maps Comparisons to observations Detectability in absorption

Lyman alpha blobs First observed by Steidel et al Redshift range z = 2 – 6.5 Observation by Matsuda et al. 2004

Cold streams

The AMR simulations Horizon MareNostrum –Ramses by Romain Teyssier –UV background: Haardt & Madau 1996 –Density dependent pressure floor: –T floor = 10 4 (n/0.1) 2/3 K for n>0.1cm -3 Ceverino, Dekel & Bournaud –Art by Andrey Kravtsov –UV background, mimics selfshielding –Gas can cool down to 100K

Computing Lyman alpha Emissivity: Collisional excitation coefficient: Case-B recombination coefficient:

More computing Number densities: Neutral Hydrogen fraction:

Lα emissivity: 50% of the gas emits Lα efficiently

Toy model: NFW profile Neistein infall (EPS) Constant infall velocity

Resulting maps: Surface brightness CDB simulation Z = 3.09 M vir = 3.5e11M O

What an observer would see: I = S / [4 π(1+z) 4 ] 0.6'' FWHM Gaussian PSF

The data for comparison:

Lyman alpha vs halo mass Several galaxies per data point z = 3.09

Luminosity function Correlation with Sheth Tormen mass function Data from Matsuda et al. 2004

Area vs. Luminosity Isophotal area above 2.2e-18 erg s -1 cm -2 arcsec -2 as a function of total luminosity

Kinematics Area vs. velocity dispersion

Energy source: Gravitational heating vs. UV background In the gas that contributes 80% of the luminosity more than 80% of the input energy is gravitational

Detectability of absorption Low sky covering fraction → difficult Low metallicity in streams→ more difficult

Resulting line profiles Lα: agreement with Steidel et al Fig. 12

Summary Cold streams loose pot. energy released as Lyman alpha photons Simulation maps very similar to observations in extent, shape, luminosity Luminosity function fits data => Cold streams can explain Lyman alpha blobs => First observational evidence for cold streams!

Thanks!