This is a composite image of N49, the brightest supernova remnant in optical light in the Large Magellanic Cloud. The Chandra X-ray image (blue) shows million-degree gas in the center. Much cooler gas at the outer parts of the remnant is seen in the infrared image from Spitzer (red). While astronomers expected that dust particles were generating most of the infrared emission, the study of this object indicates that much of the infrared is instead generated in heated gas.
The unique filamentary structure seen in the optical image by Hubble (white & yellow) has long set N49 apart from other well understood supernova remnants, as most supernova remnants appear roughly circular in visible light. Recent mapping of molecular clouds suggests that this supernova remnant is expanding into a denser region to the southeast, which would cause its asymmetrical appearance. This idea is confirmed by the Chandra data. Although X-rays reveal a round shell of emission, the X-rays also show brightening in the southeast, confirming the idea of colliding material in that area.
==Summary== This is a composite image of N49, the brightest supernova remnant in optical light in the Large Magellanic Cloud. The Chandra X-ray image (blue) shows million-degree gas in the center. Much cooler gas at the outer parts of the remnant is seen
ไฟล, sig06, ไฟล, ประว, ไฟล, หน, าท, ภาพน, การใช, ไฟล, วนกลาง, อม, ลเก, ยวก, บภาพขนาดของต, วอย, างน, กเซล, ความละเอ, ยดอ, กเซล, กเซล, กเซล, กเซล, กเซล, ภาพท, ความละเอ, ยดส, งกว, 8206, กเซล, ขนาดไฟล, เมกะไบต, ชน, ดไมม, image, jpeg, ปภาพหร, อไฟล, เส, ยงน, นฉบ, บอ. ifl prawtiifl hnathimiphaphni karichiflswnklang khxmulekiywkbphaphkhnadkhxngtwxyangni 575 600 phikesl khwamlaexiydxun 230 240 phikesl 460 480 phikesl 736 768 phikesl 982 1 024 phikesl 2 320 2 420 phikesl duphaphthimikhwamlaexiydsungkwa 8206 2 320 2 420 phikesl khnadifl 2 36 emkaibt chnidimm image jpeg rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid enuxha 1 khwamyx 2 File info 3 Individual images 4 karxnuyatichsiththi khwamyx This is a composite image of N49 the brightest supernova remnant in optical light in the Large Magellanic Cloud The Chandra X ray image blue shows million degree gas in the center Much cooler gas at the outer parts of the remnant is seen in the infrared image from Spitzer red While astronomers expected that dust particles were generating most of the infrared emission the study of this object indicates that much of the infrared is instead generated in heated gas The unique filamentary structure seen in the optical image by Hubble white amp yellow has long set N49 apart from other well understood supernova remnants as most supernova remnants appear roughly circular in visible light Recent mapping of molecular clouds suggests that this supernova remnant is expanding into a denser region to the southeast which would cause its asymmetrical appearance This idea is confirmed by the Chandra data Although X rays reveal a round shell of emission the X rays also show brightening in the southeast confirming the idea of colliding material in that area File info khaxthibaySig06 030 jpg Stellar Debris in the Large Magellanic Cloudwnthi 29 phvscikayn ph s 2549aehlngthima http gallery spitzer caltech edu Imagegallery image php image name sig06 030phusrangsrrkh X ray NASA CXC Caltech S Kulkarni et al Optical NASA STScI UIUC Y H Chu amp R Williams et al IR NASA JPL Caltech R Gehrz et al karxnuyat karichiflniihm http www spitzer caltech edu Media mediaimages copyright shtml Individual images see http gallery spitzer caltech edu Imagegallery image php image name sig06 030 High quality tif files also avaliable karxnuyatichsiththi Public domain Public domain false falsephaphniepnsatharnsmbti enuxngcakepnphaphthisrangkhunodyxngkhkarbriharkarbinaelaxwkasaehngchati NASA sungtamnoybaydanlikhsiththikhxngnasarabuiwwa phaphaelasuxtang khxngnasaimidrbkarkhumkhrxngodylikhsiththiykewncarabuiwwamilikhsiththi duephimthi hnanoybaydanlikhsiththikhxngnasa hrux noybaykarichphaphkhxng JPLkhaetuxn karich olokkhxngnasa ekhruxnghmayaelaekhruxngpradbkhxngnasa thukcakddwykdhmayshrthxemrikainlksna 14 khxngkhxbngkhbthangrachkarshrthxemrika swnthi 1221 ewbistkhxngnasaekbrwbrwmphaphthimacakxngkhkarxwkasosewiyt xngkhkarxwkasaehngchatirsesiy aelaxngkhkarxwkasthimiichxngkhkarxwkaskhxngshrthxemrika epncanwnmak phaphehlaniimcaepntxngepnsatharnsmbtiesmxip phaphhruxsuxthimacak klxngothrthrrsnxwkashbebil xacmilikhsiththi hakphaphhruxsuxnnimidrabuchdecnwamacak sthabnwithyasastrklxngothrthrrsnxwkas 1 phaphhruxsuxthnghmdthimacakekhruxngmuxkhxng okhrngkarsuksadwngxathityaelalmsuriya milikhsiththi karnaphaphhruxsuxcakokhrngkaripichnxkehnuxcakkarichephuxkarkhahruxephuxkarsuksa txngidrbxnuyatkxn 2 phaphthithukkhdeluxkihepn phaphdarasastrpracawn APOD bnewbistkhxng APOD xacmilikhsiththi 3 中文 大麦哲伦星云恒星残骸khabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairixethmthiaesdngxyuiniflniprakxbdwywnthisrang wnkxtng29 phvscikayn 2006MIME type xngkvsimage jpeg prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn03 01 12 krkdakhm 25502 320 2 420 2 36 emkaibt Anzibanonzi Summary This is a composite image of N49 the brightest supernova remnant in optical light in the Large Magellanic Cloud The Chandra X ray image blue shows million degree gas in the center Much cooler gas at the outer parts of the remnant is seen hnathimiphaphni hnatxipni oyngmathiphaphni sakmhanwdara karichiflswnklang wikixuntxipniichiflni karichbn af wikipedia org Supernova oorblyfsel karichbn ar wikipedia org بقايا مستعر أعظم karichbn ca wikipedia org Llista de romanents dels supernova karichbn da wikipedia org Supernovarest karichbn de wikipedia org Supernovauberrest Liste von Supernova Uberresten karichbn el wikipedia org LMC N49 karichbn en wikipedia org List of supernova remnants Portal Astronomy Picture Week 24 2008 LMC N49 karichbn et wikipedia org Supernoova jaanuk karichbn fa wikipedia org بازمانده ابرنواختر karichbn fi wikipedia org Luettelo supernovajaanteista karichbn he wikipedia org שארית סופרנובה karichbn hu wikipedia org Szupernova maradvany karichbn id wikipedia org Sisa sisa supernova karichbn it wikipedia org Grande Nube di Magellano Nubi di Magellano Resto di supernova N49 astronomia Portale Oggetti del profondo cielo Galleria Portale Oggetti del profondo cielo karichbn ja wikipedia org 超新星残骸 karichbn ko wikipedia org 초신성잔해 초신성잔해 목록 karichbn la wikipedia org Reliquiae supernovae karichbn lb wikipedia org Supernovarescht karichbn lt wikipedia org Supernovos liekana karichbn nl wikipedia org Supernovarest LMC N49 karichbn nn wikipedia org Supernovarest karichbn no wikipedia org Supernovarest karichbn pl wikipedia org Wikipedysta Sobi3ch galeria LMC N49 karichbn ru wikipedia org LMC N49 karichbn sk wikipedia org Portal Astronomia Obrazky tyzdna 2008 Portal Astronomia Obrazok tyzdna 24 2008 karichbn sl wikipedia org Ostanek supernove karichbn sv wikipedia org LMC N49 karichbn tr wikipedia org Supernova kalintisi karichbn uk wikipedia org Perelik zalishkiv nadnovih karichbn vi wikipedia org Tan tich sieu tan tinh karichbn zh wikipedia org LMC N49khxmulekiywkbphaph 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