Blue Halos

Spore Prints and Preparation, 248 Stropharia (Psilocybe) cubensis (San Isidro), 250 Psilocybe semilanceata (Liberty Caps), 253 Panaeolus subbalteatus (benanosis), 256 Psilocybe cyanescens (Wavy Caps, Blue Halos), 257 Psilocybe baeocystis, 258 Pilocybe stuntzii, 260... 

Psilocybe cyanescens (Wavy Caps, Blue Halos)... 

Discussion—When the ignition source is a test flame, the application of the test flame may cause a blue halo or an enlaigM flame prior to the actual flash point This is not a flash and should be ignored. 

Fig. 1. Variation in [Fe/H] versus Galactic rotational velocity for stars assigned to Galactic stellar populations based purely on their kinematics thin disk (red), thick disk (green), halo (cyan), plunging orbits (blue), extreme retrograde orbits (black).

The offsets of axes determine the characteristic mass Me that constrains supernova debris and the true yield y (p in the text). MB is the corresponding blue absolute magnitude (neglecting any dark halos). The trend along the linear branch of the curve is for metallicity to increase approximately as A/1/2. After Lynden-Bell (1992). 

Fig. 13.2. Illustration of the basic concept of Basis Products, (a) The PGVL reaction scheme of VRXN-2-00051 (formation of the H-imidazo[1,2-a]pyridine ring system using aminoheterocycles and alpha-halo ketones) is used for the illustration (b) The Basis Products of A are formed by all A reactants with one constant reactant (B CAP, 1 -bromopropan-2-one). The Basis products of are formed by all reactants with a constant A reactant (A CAP, 2-amino pyridine). The blue triangle and yellow hexagon represent two such basis products. The red star represents a product molecule which is related to those two corresponding basis products.

Figure 5.3. Left. The gamma-ray emission from XX annihilation in a rich, Coma-like, nearby galaxy cluster is shown Mx = 70 — 500 GeV (from top down). The integral flux is compared to the sensitivity of ongoing and planned gamma-ray experiments, as labelled. Right. The diffuse synchrotron emission spectrum of secondary electrons produced in XX annihilation is shown to fit the Coma radio-halo spectrum the green area represent the prediction of a model in which the x annihilates predominantly into fermions, while the blue area represent the gauge-boson dominated x annihilation (from Colafrancesco Mele 2001).

Figure 5.4. Left. The overall SZ effect in Coma produced by the combination of various electron populations thermal hot gas with ksT = 8.2 keV and r = 4.9 10-3 (solid blue curve) which best fits the available SZ data relativistic electrons which best fit the radio-halo spectrum (yellow curve) provide a small additional SZ effect (Colafrancesco 2004a) warm gas with ksT v 0.1 keV and n 10-3 cm-3 (cyan curve) provides a small SZ effect due to its low pressure (Colafrancesco 2004c) DM produced secondary electrons with Mx = 10 (black dotted curve), 20 GeV (black solid curve) and 30 GeV (dashed solid curve). A pure-gaugino x reference model is assumed in the computations. The relative overall SZ effect is shown as the dotted, solid and dashed red curves, respectively. A zero peculiar velocity of Coma is assumed consistently with the available limits. SZ data are from OVRO (magenta), WMAP (cyan) and MITO (blue). Right. The constraints on the

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