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ropoto · 1 year

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PENELOPE GARCIA | SEASON 3

#penelope garcia #criminal minds #criminalmindsedit #cm #cm 3x02 #cm 3x03 #cm 3x04 #cm 3x06 #cm 3x08 #cm 3x10 #cm 3x14 #cm 3x15 #cm 3x17 #cm 3x18

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damnhotmsimmons · 9 months

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Endless gifs of Jennifer Jareau

True Night-3x10

#jennifer jareau #criminal minds #criminalmindsverse #criminalmindsedit #smallscreensource #filmtvcentral #userthing #usercrime #my gifs #my edit #cmedit #cm 3x10 #aj cook

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idiotlovers · 1 year

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PENELOPE GARCIA in SEASON 3

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stephsycamore · 6 months

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Back to mt regularly scheduled programming.

S3 ep 10 true night! I know people love this episode and it is really good and visually so distinct from the other episodes but its just not my thing lol

Also is it ever explained how malcolm in the middle skinny comic book writer is able to kill all these armed gang members with a goddamn sword?? Is he on meth?? Or does his delusion give him super strength?? Killing people with a sword is really physical??

Also the bit with garcia and morgan at the beginning is so cute.

#criminal minds #penelope garcia #derek morgan #cm 3x10

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spencersweatervest · 2 years

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the way they played heroes on the episode garcia almost died & on the episode she left

#criminal minds #penelope garcia #spencer reid #emily prentiss #derek morgan #jennifer jareau #aaron hotchner #david rossi #jason gideon #elle greenaway #aaron hotch hotchner #tara lewis #matthew simmons #matt simmons #luke alvez #cm 15x10 #cm 3x10 #3x10 cm #criminal minds: mine

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marril96 · 1 year

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Criminal Minds 3.10 | True Night

#derek morgan #spencer reid #jennifer jareau #jj #cm #criminal minds #cmedit #criminalmindsedit #tusergabs #fieryfrankie #mgg #matthew gray gubler #shemar moore #aj cook #a.j. cook #3x10 #true night #my gifs #edit

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maschotch · 2 years

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#3x10 #penelope garcia #cm caps

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starrynyxa · 1 year

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they fr went all out for the props for this episode. the comic strips and drawings look sick as hell

#cm lb #3x10

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artsofrajasthanindia · 24 days

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Beautiful White handmade Cotton block print rug weaved on Indian looms stamped with natural vegetable-dyes using hand-made wooden blocks achieving the perfection of block printing art of Jaipur. This is best suitable for your home office entrance, bedroom, living room, kids’ room, dining room, kitchen and outdoor patio, terrace, beach and garden.

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carlosviloriadesign · 2 years

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Hanging 5 Split Panel Canvas Mockup - 30x100x2.8 cm

5 Split Panel Canvas Mockup, the tool you need to divide any landscape image into 5 pieces of canvas with ratios 3x10 - 30x100x3 cm - 50% Discount For Limit Time - $12

5 Split Panel Canvas Mockup, the tool you need to divide any landscape image into 5 pieces of canvas with ratios 3×10 – 30x100x2.8 cm, showcase any photography or digital artworks as a photo-realistic printed 5 Split Canvas to sell in your print store. Easy to edit using smart objects for Photoshop, it also has some details that make it more realistic, change the opacity of the brightness and…

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kreuzaderny · 2 years

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A Cool Accretion Disk around the Galactic Centre Black Hole

A supermassive black hole SgrA* with the mass ~4x10^6 Msun resides at the centre of our galaxy. Building up such a massive black hole within the ~10^10 year lifetime of our galaxy would require a mean accretion rate of ~4x10^-4 Msun/yr. At present, X-ray observations constrain the rate of hot gas accretion at the Bondi radius (10^5 R_Sch = 0.04 pc at 8kpc) to \dot{M}_Bondi ~ 3x10^-6 Msun/yr, and polarization measurements constrain it near the event horizon to \dot{M}_horizon ~ 10^{-8} Msun/yr. A range of models was developed to describe the accretion gas onto an underfed black hole. However, the exact physics still remains to be understood. One challenge with the radiation inefficient accretion flows is that even if one understands the dynamics there is no accepted prescription for associating emissivity (and absorption) with the flow. The other issue is the lack of model-independent probes of accretion flow at intermediate radii (between few and ~ 10^5 R_Sch), i.e. the constraints that do not assume a model of accretion flow as an input parameter. We report detection and imaging of the 10^4 K ionized gas disk within 2x10^4 R_Sch in a mm hydrogen recombination line H30alpha: n = 31 -> 30 at 231.9 GHz using the ALMA. The emission was detected with a double-peaked line profile spanning full width of 2,200 km/s with the approaching and the receding components straddling Sgr A*, each offset from it by 0.11arcsec= 0.004pc. The red-shifted side is displaced to the north-east, while the blue-shifted side is displaced to the south-west. The limit on the total mass of ionized gas estimated from the emission is 10^-4 - 10^-5 Sun at a mean hydrogen density 10^5-10^6 cm^-3, depending upon whether or not we assume the presence of a uniform density disk or an ensemble of orbiting clouds, and the amplification factor of the mm radiation due to the strong background source which is Sgr A* continuum.

#astronomy #space #black hole

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ropoto · 2 years

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