সারাংশ

This image from NASA's Spitzer Space Telescope transforms a dark cloud into a silky translucent veil, revealing the molecular outflow from an otherwise hidden newborn star. Using near-infrared light, Spitzer pierces through the dark cloud to detect the embedded outflow in an object called HH 46/47. Herbig-Haro (HH) objects are bright, nebulous regions of gas and dust that are usually buried within dark clouds. They are formed when supersonic gas ejected from a forming protostar, or embryonic star, interacts with the surrounding interstellar medium. These young stars are often detected only in the infrared.

The Spitzer image was obtained with the infrared array camera. Emission at 3.6 microns is shown as blue, emission from 4.5 and 5.8 microns has been combined as green, and 8.0 micron emission is depicted as red.

HH 46/47 is a striking example of a low mass protostar ejecting a jet and creating a bipolar, or two-sided, outflow. The central protostar lies inside a dark cloud (known as a 'Bok globule') which is illuminated by the nearby Gum Nebula. Located at a distance of 1140 light-years and found in the constellation Vela, the protostar is hidden from view in the visible-light image (inset). With Spitzer, the star and its dazzling jets of molecular gas appear with clarity.

The 8-micron channel of the infrared array camera is sensitive to emission from polycyclic aromatic hydrocarbons. These organic molecules, comprised of carbon and hydrogen, are excited by the surrounding radiation field and become luminescent, accounting for the reddish cloud. Note that the boundary layer of the 8-micron emission corresponds to the lower right edge of the dark cloud in the visible-light picture.

Outflows are fascinating objects, since they characterize one of the most energetic phases of the formation of low-mass stars (like our Sun). The jets arising from these protostars can reach sizes of trillions of miles and velocities of hundreds of thousands miles per hour. Outflows are clear evidence of the presence of a process that creates supersonic beams of gas. This mechanism is tightly bound to the presence of circumstellar discs which surround the young stars. Such discs are likely to contain the materials from which planetary systems form. Our Sun probably underwent a similar process some 4.5 billion years ago. Hence the interest in understanding how quickly and efficiently this mass accretion and loss process takes place in protostars.

মূল আপলোড লগ

এটি একটি পুনঃসম্পাদিত চিত্র, যার মানে হল যে এটি ডিজিটালরূপে এটির মূল সংস্করণ থেকে পরিবর্তন করা হয়েছে। পরিবর্তন: Czech translation। আসলটি দেখা যাবে এখানে: Ssc2003-06f.jpg। Jan.Kamenicek কর্তৃক এটি পরিবর্তিত হয়েছে।

	এই ফাইলটি পাবলিক ডোমেইনে আছে কারণ এটি শুধুমাত্র নাসা কর্তৃক নির্মিত হয়েছিল। নাসার কপিরাইট নীতি হচ্ছে যে "নাসা কর্তৃক উল্লেখ না থাকলে নাসার উপাদান কপিরাইট দ্বারা সুরক্ষিত নয়"। (Template:PD-USGov, নাসার কপিরাইট নীতির পাতা অথবা জেপিএল চিত্র ব্যবহারের নীতি দেখুন।)
	সতর্কবার্তা: Use of NASA logos, insignia and emblems are restricted per US law 14 CFR 1221. The NASA website hosts a large number of images from the Soviet/Russian space agency, and other non-American space agencies. These are not necessarily in the public domain. Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI.[1] See also {{PD-Hubble}} and {{Cc-Hubble}}. The SOHO (ESA & NASA) joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use. [2] Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. [3]

মূল আপলোড লগ

This image is a derivative work of the following images:

• File:Ssc2003-06f.jpg licensed with PD-USGov-NASA
  • 2007-07-05T21:12:22Z Anzibanonzi 1500x1200 (1013912 Bytes) This image from NASA's Spitzer Space Telescope transforms a dark cloud into a silky translucent veil, revealing the molecular outflow from an otherwise hidden newborn star. Using near-infrared light, Spitzer pierces through t

Uploaded with derivativeFX