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Those of us that are born under the Gemini sign can sometimes get a reputation for being a bit, well, all over the place. But there’s actually a lot more to the Gemini personality than many realize and they possess many unique traits and characteristics that often aren’t noticed at first glance.
So to give you an idea of what it really means to be a Gemini lets take a look at 21 of the most common traits and characteristics of the Gemini personality.
1. Gemini tries to avoid conflict and will walk away before things get too heated.
The Gemini tries to avoid pointless drama and conflict and when possible will simply walk away from a tense situation before things get too heated.
They’ve got more important things to focus on and they’d much rather just forget about it and get on with life.
2. But if you force Gemini into a corner they will not hesitate to retaliate.
Gemini tries to be a pacifist but if you back them into a corner and leave them no other option then they will not hesitate to retaliate and put you in your place.
They’re not afraid to stand up for themselves and can be quite cutting with their words when they are angry.
3. Gemini is a fiercely loyal friend, ally and lover.
Whether it’s friends, family or a lover the Gemini tends to be extremely loyal once they have committed to someone.
They can be picky about who they give their trust to but those who have earned it will have an ally in Gemini for life.
4. The Gemini mind is constantly racing with thoughts and ideas.
The mind of the Gemini is constantly racing and contemplating all sorts of thoughts, ideas and questions.
They are naturally curious about practically everything and can find it hard to stick to any one thing for too long because their passions and interests are so diverse.
5. Gemini is extremely independent and can’t be controlled.
Geminis tend to be extremely independent and self reliant and they like to forge their own path in life rather than live in someone else’s shadow.
They need the freedom to be able to live life on their own terms and if you are trying to control them or ‘box them in’ then they will be quick to distance themself from you.
6. Gemini is observant as hell and constantly soaking up knowledge.
The Gemini is a curious creature who is constantly observing their surroundings and soaking up knowledge everywhere that they go.
They are natural investigators with a knack for figuring out the truth… never underestimate their ability to get to the bottom of things!
7. Gemini can be an outrageous flirt at times.
Geminis have a habit of being massive flirts sometimes. They can’t help it though and half the time they don’t even realize they are doing it.
They’re just naturally friendly people who have a real way with words.
8. Gemini has no patience for overly critical people that do nothing but complain.
Jetbrains phpstorm 2 1 2 ubkg download free. Gemini has little-to-no time for serial complainers who insist on poking holes in absolutely everything.
If you sound like a broken record just whining about same things over and over and over and over again… then they will get bored and find somebody else to hang out with.
9. Gemini is drawn to people who can stimulate their mind.
Gemini can’t get enough of people that can stimulate their mind and they find themselves drawn towards those that have witty banter, interesting stories and an ability to make them laugh.
They love it when they find someone that’s on their wavelength and that they can bounce ideas off of.
10. Gemini is NOT afraid to tell you exactly what they think.
The Gemini has got a lot of opinions and you better believe that they are going to share them with with the world.
They’re the kinds of people that will tell you exactly what is on their mind without any kind of filter… even if it’s not pretty.
11. Gemini is a supportive and encouraging friend.
When one of their friends or loved ones has problems the Gemini often picks up on it instinctively before a word is even said about it… and they will then go out of their way to make sure they are okay.
They always know exactly what to say to make someone feel better and are great at giving advice that is actually helpful.
![Descaling Descaling](https://i.pinimg.com/originals/9f/2e/ae/9f2eae4860b8660ebcb1aaa720ec7ba1.jpg)
12. Gemini can be a bit of a weirdo sometimes.
Gemini can be random, unpredictable and a downright weirdo at times leaving others perplexed and wondering just what the the hell it is that they’re going to do next.
They aren’t big fans of anything too dull and ordinary and prefer to constantly mix things up and go against the grain. One thing is for sure… with Gemini around you will never be bored.
13. Gemini knows how to smooth talk their way into just about anything.
Geminis are extremely articulate and surprisingly persuasive when they want to be.
They have an uncanny ability to talk someone into almost anything… and can even make them think that it was their own idea in the first place!
14. Gemini is restless and always on the go.
Gemini doesn’t like to stay in any one place for too long and they tend to be always on the go and on some mission or another.
They have a restless soul that craves new experiences and they can feel suffocated by too much repetition and routine.
15. Gemini is driven by curiosity and soaks up knowledge like a sponge.
![Gemini Gemini](https://www.reginamarine.com/wp-content/uploads/2019/04/IMG_8215-1024x768.jpg)
The Gemini is an extremely curious creature who can’t help but be inquisitive about practically everything.
They tend to be constantly soaking up knowledge like a sponge and are they’re always looking to discover new things.
16. Gemini can experience EXTREME emotions.
The Gemini personality is prone to experiencing intense emotions… both good and bad.
These emotional traits and characteristics mean that their highs can be amazing but their lows can be just as extreme and leave them feeling emotionally exhausted.
17. Gemini can be guarded and reluctant to ‘open up’.
The Gemini loves to talk but if you bring up something that’s too personal they may just suddenly put up a wall and avoid the topic altogether.
Sometimes they get a bit defensive particularly if they aren’t sure if they can trust you yet.
18. Gemini can take their time to commit to a relationship but once they do they go ‘all in’.
The Gemini can be somewhat reluctant to commit to any one person but when they do finally take the plunge they they make sure to give the relationship everything that they’ve got.
They tend to be very ‘all or nothing’ kinds of lovers and once they’re in a relationship they are an incredibly loyal partner.
19. Gemini has a wild and adventurous spirit.
Whether it comes to their career, hobbies, love life or anything else… the Gemini likes to be adventurous in everything that they do.
They like to take the scenic route in life and are almost always up for doing something a bit crazy.
20. Gemini has a wickedly sarcastic sense of humor.
The Gemini has a sharp wit and they are well known for their extremely dry and sarcastic sense of humor.
Their jokes may fly right over people heads of some but those that can actually keep up with their train of thought often find them hilarious.
21. Gemini is adaptable and able to roll with the punches.
The Gemini is well know for being one of the most versatile and adaptable personalities in all of the zodiac and they can adjust to new surroundings and circumstances a lot faster than many of the other signs.
When the shit hits the fan they’re more than capable of rolling with the punches no matter what life throws their way!
The central ~30 arcseconds of the galaxy Centaurus A (one arcsecond ~ 55 light-years). The contours are the mid-infrared emission at 8.8 microns from the Gemini data and processed to highlight the low-level extended emission. The color HST image shows the Paschen-alpha emission from Marconi et al. 2000, ApJ, 528, 276 which primarily traces regions of star formation. The dotted line represents the axis of the powerful radio jet emanating from the supermassive black hole perpendicular to the torus. Full resolution image available here.
Embargoed until 9:20 AM (Pacific Time), Tuesday, January 9, 2007
Science Contacts:
- Dr. James Radomski
Gemini Observatory, La Serena, Chile
+56-51-205-640 (desk)
[email protected] - Dr. Christopher Packham
University of Florida, Gainsville, FL
(352) 392-2052 (desk)
(352) 514-3333 (cell)
[email protected]
Media Contact:
- Peter Michaud
Gemini Observatory, Hilo HI, USA
(808) 974-2510 (desk)
(808) 937-0845 (cell)
[email protected]
www.gemini.edu
Fundamental to theories describing active galactic nuclei (AGN) is the prediction that a doughnut-shaped ring of material (a torus) surrounds a supermassive black hole in these energetic galactic cores. Yet, understanding an AGN's torus, or indeed seeing one directly, has proved to be extremely frustrating, and has spurred an ongoing debate about their extent and physical properties.
To help settle the debate, an international team of astronomers used a novel approach to peer deeply into the energetic core of the nearby galaxy Centaurus A. Their observations didn't resolve the theoretical torus, but did set stringent constraints on its size and characteristics, indicating that it is likely quite petite and clumpy.
These results were presented today at the 209th meeting of the American Astronomical Society meeting in Seattle, Washington.
The team used observations made at mid-infrared wavelengths with the 8-meter Gemini South telescope in Chile to study warm dust in the nucleus of the galaxy Centaurus A. The results indicate that the theorized doughnut-shaped torus thought to exist at the core of this nearby AGN is beyond the resolution of the largest non-interferometric ground-based telescopes and therefore must be smaller than many models predicted. Team members used an innovative statistical analysis technique and high-resolution images to establish extremely tight constraints on the size of the warm dust in the torus. 'We think that this data provides the strongest argument yet in constraining the maximum size of the warm dusty torus in a galaxy of this type,' said Principal Investigator and Gemini Observatory astronomer James Radomski.
The research team obtained these observations with the mid-infrared instrument T-ReCS to help settle the ongoing debate about whether the torus and central regions of Centaurus A were ever resolved in previous observations. 'If the torus had been resolved in previous observations, that would mean that the extent of the torus is much larger than the latest models predict, and it would have left many of us scratching our heads,' said team member Chris Packham of the University of Florida.
Earlier observations made with the 10-meter Keck I telescope by D. Whysong (now at NRAO) and R. Antonucci (University of California, Santa Barbara, with Whysong when this work was done) initially proposed a similar resolution-limited size for the torus in Centaurus A. However, a team using the Magellan Telescope subsequently claimed that the nucleus was indeed resolved and therefore indicative of a much larger structure. The new Gemini South result clearly confirms the earlier Keck result by Whysong and Antonucci.
'This debate definitely shows the difficulty of making these types of observations,' said Radomski. 'But these observations are critical since we cannot understand the environments around a supermassive galactic black hole without first knowing the extent of its torus.'
The new theoretical models of a galactic torus helps to settle what some were calling the 'torus size crisis.' Without such a model, the observations of Centaurus A would have deepened the size crisis. 'These more recent models predict that, far from being a huge and uniform doughnut of gas and dust as once thought, instead the torus orbits the supermassive black hole in clumps. The size constraints placed by the Keck and Gemini data indicate that the clumps are primarily 'bunched up' and must orbit within a few light-years of the black hole,' explained team member Nancy Levenson of the University of Kentucky.
Unlike with previous observations, the Gemini team cross-calibrated the mid-infrared data many times against a reference star in order to determine with a high degree of certainty that the nucleus of Centaurus A was unresolved. In addition, because the object was observed for long periods of time, these observations were deep enough to probe the very faint emission beyond the nucleus previously observed only by space based observatories such as the Spitzer Space Telescope. However, Gemini's larger aperture provided higher spatial resolution to reveal details in these regions thought to be due to star formation. It may also trace emission from material flowing into and feeding the black hole at the center of the galaxy.
'By working with a combination of instrument builders, observational and theoretical astronomers, this work has pooled the knowledge of an international group of astronomers in order to gain insights into these objects and extract the maximum amount of knowledge from hard-won telescope time to produce this convincing result,' said team member Chris Packham of University of Florida.
Team members (listed by institution) are James T. Radomski, James M. DeBuizer, and Rachel Mason (Gemini Observatory), Christopher Packham, Charles M. Telesco, Manuel Orduna (University of Florida), N.A. Levenson (University of Kentucky), Eric Perlman (University of Maryland), Lerothodi L. Leeuw (Rhodes University, South Africa), and Henry Matthews (Herzberg Institute of Astrophysics, Canada).
The central ~30 arcseconds of the galaxy Centaurus A (one arcsecond ~ 55 light-years). The contours are the mid-infrared emission at 8.8 microns from the Gemini data and processed to highlight the low-level extended emission. The color HST image shows the Paschen-alpha emission from Marconi et al. 2000, ApJ, 528, 276 which primarily traces regions of star formation. The dotted line represents the axis of the powerful radio jet emanating from the supermassive black hole perpendicular to the torus. Full resolution image available here.
Diminuta y tibia rosquilla alimenta Teorías de Agujeros Negros Extragalácticos
Contactos Científicos:
- Dr. James Radomski
Gemini Observatory, La Serena, Chile
+56-51-205-640 (oficina)
[email protected] - Dr. Christopher Packham
University of Florida, Gainsville, FL
(352) 392-2052 (oficina)
(352) 514-3333 (celular)
[email protected]
Contacto para Prensa:
- Peter Michaud
Gemini Observatory, Hilo HI, USA
(808) 974-2510 (oficina)
(808) 937-0845 (celular)
[email protected]
www.gemini.edu - Ma. Antonieta García
Gemini Observatory, La Serena, Chile
(56) 51- 205628 (oficina)
(56) 99182858 (celular)
La predicción sobre la existencia de un anillo de material (torus) en forma de rosquilla que rodea a un agujero negro super masivo en los núcleos energéticos galácticos, resulta fundamental para las teorías que describen un núcleo galáctico activo (AGN por sus siglas en inglés). Más aún, el poder comprender un torus de un AGN o incluso el ver uno directamente, es extremadamente frustrante, y ha estimulado un constante debate sobre su extensión y sus propiedades físicas. Focus 1 8 9.
Para ayudar a coordinar el debate, un equipo internacional de astrónomos utilizó un acercamiento de novela para emparejar profundamente en el centro energético de la Galaxia cercana Centauro A. Sus observaciones no resolvieron el torus teórico, pero si se fijaron rigurosas restricciones en relación a su tamaño y características, indicando que es más bien pequeña y torpe.
Los resultados fueron presentados en la reunión 209 de la Sociedad Norteamericana de Astronomía en Seattle, Estados Unidos.
El equipo utilizó observaciones realizadas en longitudes de onda del infrarrojo medio con el Telescopio de 8 metros de Gemini Sur en Chile con el fin de estudiar el polvo tibio en el núcleo de la galaxia Centaurus A. Los resultados indican que el torus en teórica forma de rosquilla que se pensaba existía en centro de su cercano AGN se encuentra más allá de la resolución de los telescopios más grandes no interferométricos desde el suelo. Por tanto, debe ser más pequeño que mucho de los modelos que se habían predecido con anterioridad. Los miembros del equipo utilizaron una técnica innovadora de análisis estadístico e imágenes de alta resolución para establecer fuertes restricciones sobre el tamaño del polvo tibio de torus. “Pensamos que estos datos brindan uno de los más fuertes argumentos al restringir el tamaño máximo de un torus polvoriento y tibio en una galaxia de este tipo,” dijo el Investigador Principal, astrónomo del Observatorio Gemini en Chile James Radomski.
El equipo de investigación obtuvo estas observaciones con el instrumento para mediano infrarrojo T-ReCS con el fin de contribuir a definir el constante debate sobre si torus y las regiones centrales de Centaurus A fueron alguna vez resueltas en observaciones previas. “Si el torus se hubiera resuelto en observaciones anteriores, eso significaría que la extension de torus es mucho más grande que los últimos modelos que se predijeron, y nos habría dejado a varios de nosotros rascando nuestras cabezas,” manifesto el integrante del equipo Chris Packham de la Universidad de Florida.
Observaciones previas realizadas con el telescopio de 10 metros Keck I a cargo de D. Whysong (ahora en NRAO) y R. Antonucci (University of California, Santa Barbara, con Whysong cuando su trabajo había concluído) inicialmente propusieron un tamaño de resolución similar para el torus en Centaurus A. De todas maneras, un equipo al utilizar el Telescopio de Magallanes subsecuentemente declaró que el núcleo esta de hecho resuelto y por tanto era indicador de una estructura mucho más grande. El nuevo resultado de Gemini Sur claramente confirma la observación hecha tempranamente con Keck por Whysong y Antonucci.
Gemini 221 Nespresso Descale Instructions
“Este debate muestra definitivamente la dificultad de hacer este tipo de observaciones “, señala Radomski. “Pero estas observaciones son críticas ya aque nosotros no podemos entender el medio ambiente que rodea a un agujero negro galactico super masivo sin primero conocer la extensión de torus.”
Los nuevos modelos teóricos de un torus galáctico nos ayudan a calmar lo que algunos llaman la “crisis de tamaño de torus.” Sin ese modelo, las observaciones de Centaurus A habrían profundizado esta crisis. “Estos modelos más recientes preveen que, lejos de ser una rosquilla grande y uniforme de gas y polvo como se pensó alguna vez, torus orbita el agujero super masivo en grupos. Las restricciones de tamaño entregadas por los datos de Keck y Gemini indican que los grupos están primariamente ‘amontonados’ y deben orbitar dentro de unos pocos años luz del agujero negro,” explicó el integrante del equipo Nancy Levenson de la Universidad de Kentucky.
A diferencia de observaciones anteriores, el equipo contra calibró los datos del mediano infrarrojo muchas veces contra una estrella de referencia para poder determinar con un alto nivel de certeza que el núcleo de Centaurus A no estaba resuelto. Además, ya que el objeto fue observado por largos períodos de tiempo , estas observaciones fueron suficientemente profundas para comprobar las pálidas emisiones más allá del núcleo previamente observado sólo desde observatorios espaciales como el Spitzer Space Telescope. De todas maneras, la gran apertura de Gemini brindó mayor resolución espacial revelando detalles en estas regiones que se pensaba eran debido a la formación estelar. También puede registrar la emisión desde dentro del flujo de material y alimentando al agujero negro en el centro de la galaxia.
“Por el hecho de trabajar con una combinación de quienes construyen instrumentos y con astrónomos teóricos y observacionales, este trabajo ha compartido el conocimiento de un grupo internacional de astrónomos para obtener instrospectivas sobre estos objetos y extraer el máximo de conocimiento del tiempo de observación en los telescopios más difíciles de conseguir con el objeto de producir este convincente resultado,” dijo el integrante del equipo Chris Packham de la Universidad de Florida.
How To Descale The Gemini 221
Los miembros del equipo (ordenados por institución) are James T. Radomski, James M. DeBuizer y Rachel Mason (Gemini Observatory), Christopher Packham, Charles M. Telesco, Manuel Orduna (Universitdad de Florida), N.A. Levenson (Universidad de Kentucky), Eric Perlman (Universidad de Maryland), Lerothodi L. Leeuw (Rhodes University, Sud Africa) y Henry Matthews (Instituto de Astrofísica Herzberg, Canada).