N44 is an emission nebula with superbubble structure located in the Large Magellanic Cloud, a satellite galaxy of the Milky Way in the constellation Dorado.[3][4][5] Originally catalogued in Karl Henize's "Catalogue of H-alpha emission stars and nebulae in the Magellanic Clouds" of 1956, it is approximately 1,000 light-years wide and 160,000-170,000 light-years distant.[6][7][1] N44 has a smaller bubble structure inside known as N44F. The superbubble structure of N44 itself is shaped by the radiation pressure of a 40-star group located near its center; the stars are blue-white, very luminous, and incredibly powerful.[6][1] N44F has been shaped in a similar manner; it has a hot, massive central star with an unusually powerful stellar wind that moves at 7 million kilometers per hour. This is because it loses material at 100 million times the rate of the Sun, or approximately 1,000,000,000,000,000 tons per year. However, varying density in the N44 nebula has caused the formation of several dust pillars that may conceal star formation.[6] This variable density is likely caused by previous supernovae in the vicinity of N44; many of the stars that have shaped it will eventually also end as supernovae. The past effects of supernovae are also confirmed by the fact that N44 emits x-rays.[4][8]
Picture combining views of N44 in visible light with images in infrared light and X-rays.[2]
N44 is classified as an emission nebula because it contains large regions of ionized hydrogen. However, the three strongest emission lines in the nebula are singly ionized oxygen atoms, which emit at an ultraviolet wavelength of 372.7 nm, doubly-ionized oxygen atoms, which emit at a blue-green wavelength of 500.7 nm, and neutral hydrogen atoms, which emit the hydrogen-alpha line at a red wavelength of 656.2 nm.[1][9]
Galleryedit
Amateur astronomer Ha/OIII/SII photo of N44
Referencesedit
^ abcd"Roses in the Southern Sky". ESO. 3 November 2003. Retrieved 7 May 2012.
^"A Surprising Superbubble". ESO Picture of the Week. Retrieved 3 September 2012.
^H. Nakajima (26 September 2005). (PDF). The X-Ray Universe Symposium. H. Yamaguchi, M. Ueno, A. Bamba, and K. Koyama. European Space Agency. Archived from the original (PDF) on 14 July 2014. Retrieved 10 May 2012.
^ abNemiroff, R.; Bonnell, J., eds. (6 February 2006). "The N44 Superbubble". Astronomy Picture of the Day. NASA. Retrieved 10 May 2012.
^Michaud, Peter (4 January 2006). "Gemini Looks Down the Mouth of an Interstellar Cavern". Gemini Observatory. Retrieved 10 May 2012.
^ abcWilkins, Jamie; Dunn, Robert (2006). 300 Astronomical Objects: A Visual Reference to the Universe (1st ed.). Buffalo, New York: Firefly Books. ISBN978-1-55407-175-3.
^"N44 in the Large Magellanic Cloud (Central Region)". ESO. 3 November 2003. Retrieved 7 May 2012.
^"Detail of N44 in the Large Magellanic Cloud". ESO. 22 June 1999. Retrieved 7 May 2012.
^Nemiroff, R.; Bonnell, J., eds. (13 February 2006). "The N44 Emission Nebula". Astronomy Picture of the Day. NASA. Retrieved 7 May 2012.
External linksedit
Media related to N44 at Wikimedia Commons
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emission, nebula, other, uses, emission, nebula, with, superbubble, structure, located, large, magellanic, cloud, satellite, galaxy, milky, constellation, dorado, originally, catalogued, karl, henize, catalogue, alpha, emission, stars, nebulae, magellanic, clo. For other uses see N44 N44 is an emission nebula with superbubble structure located in the Large Magellanic Cloud a satellite galaxy of the Milky Way in the constellation Dorado 3 4 5 Originally catalogued in Karl Henize s Catalogue of H alpha emission stars and nebulae in the Magellanic Clouds of 1956 it is approximately 1 000 light years wide and 160 000 170 000 light years distant 6 7 1 N44 has a smaller bubble structure inside known as N44F The superbubble structure of N44 itself is shaped by the radiation pressure of a 40 star group located near its center the stars are blue white very luminous and incredibly powerful 6 1 N44F has been shaped in a similar manner it has a hot massive central star with an unusually powerful stellar wind that moves at 7 million kilometers per hour This is because it loses material at 100 million times the rate of the Sun or approximately 1 000 000 000 000 000 tons per year However varying density in the N44 nebula has caused the formation of several dust pillars that may conceal star formation 6 This variable density is likely caused by previous supernovae in the vicinity of N44 many of the stars that have shaped it will eventually also end as supernovae The past effects of supernovae are also confirmed by the fact that N44 emits x rays 4 8 N44Emission nebulasuperbubbleThe central region of N44Observation data J2000 0 epochRight ascension6 29hDeclination 61 36 Distance 160 000 170 000 lyConstellationDoradoPhysical characteristicsRadius 500 1 lySee also Lists of nebulae Picture combining views of N44 in visible light with images in infrared light and X rays 2 N44 is classified as an emission nebula because it contains large regions of ionized hydrogen However the three strongest emission lines in the nebula are singly ionized oxygen atoms which emit at an ultraviolet wavelength of 372 7 nm doubly ionized oxygen atoms which emit at a blue green wavelength of 500 7 nm and neutral hydrogen atoms which emit the hydrogen alpha line at a red wavelength of 656 2 nm 1 9 Gallery edit nbsp Amateur astronomer Ha OIII SII photo of N44References edit a b c d Roses in the Southern Sky ESO 3 November 2003 Retrieved 7 May 2012 A Surprising Superbubble ESO Picture of the Week Retrieved 3 September 2012 H Nakajima 26 September 2005 Exploring High Energy Activities in the Superbubble N44 With XMM NEWTON PDF The X Ray Universe Symposium H Yamaguchi M Ueno A Bamba and K Koyama European Space Agency Archived from the original PDF on 14 July 2014 Retrieved 10 May 2012 a b Nemiroff R Bonnell J eds 6 February 2006 The N44 Superbubble Astronomy Picture of the Day NASA Retrieved 10 May 2012 Michaud Peter 4 January 2006 Gemini Looks Down the Mouth of an Interstellar Cavern Gemini Observatory Retrieved 10 May 2012 a b c Wilkins Jamie Dunn Robert 2006 300 Astronomical Objects A Visual Reference to the Universe 1st ed Buffalo New York Firefly Books ISBN 978 1 55407 175 3 N44 in the Large Magellanic Cloud Central Region ESO 3 November 2003 Retrieved 7 May 2012 Detail of N44 in the Large Magellanic Cloud ESO 22 June 1999 Retrieved 7 May 2012 Nemiroff R Bonnell J eds 13 February 2006 The N44 Emission Nebula Astronomy Picture of the Day NASA Retrieved 7 May 2012 External links edit nbsp Media related to N44 at Wikimedia Commons nbsp This nebula related article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title N44 emission nebula amp oldid 1211035807, wikipedia, wiki, book, books, library,
