MCG+07-33-027 is an isolated spiral galaxy located about 330 million light-years away in the constellation Hercules. It has a very high rate of star formation which would make it a starburst galaxy. Normally, starburst galaxies are triggered by the collision of another galaxy. However most galaxies are in groups or clusters, while MCG+07-33-027 is solitary. Therefore, the cause of the starburst was not due to a collision or by the passing of a nearby galaxy and so the cause of the activity remains unknown. On April 2, 2005, SN 2005bk, a supernova of type Ic was discovered in MCG+07-33-027.
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| - MCG+07-33-027 (ar)
- MCG+07-33-027 (it)
- MCG+07-33-027 (en)
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| - MCG+07-33-027 هي مجرة حلزونية منعزلة تقع على بعد 330 مليون سنة ضوئية في كوكبة الجاثي. تمتلك نسبة عالية جداً من تشكيل النجوم التي من شأنها أن تجعل من المجرة مجرة انفجار نجمي. عادةً، المجرات تنفجر بسبب اصطدام مجرة أخرى. ومع ذلك معظم المجرات هي في مجموعات أو تجمعات عنقودية، في حين أن مجرة MCG+07-33-027 انفرادية. لذلك، فإن سبب الإنفجار لم يكن بسبب الاصطدام أو بمرور مجرة مجاورة، وبالتالي فإن سبب النشاط لا يزال مجهولاً. (ar)
- MCG+07-33-027 is an isolated spiral galaxy located about 330 million light-years away in the constellation Hercules. It has a very high rate of star formation which would make it a starburst galaxy. Normally, starburst galaxies are triggered by the collision of another galaxy. However most galaxies are in groups or clusters, while MCG+07-33-027 is solitary. Therefore, the cause of the starburst was not due to a collision or by the passing of a nearby galaxy and so the cause of the activity remains unknown. On April 2, 2005, SN 2005bk, a supernova of type Ic was discovered in MCG+07-33-027. (en)
- MCG+07-33-027 è una galassia a spirale (S0) situata nella costellazione di Ercole alla distanza di oltre 330 milioni di anni luce dalla Terra. L'immagine raccolta dal Telescopio spaziale Hubble ci mostra la galassia vista di faccia (face-on). Nel 2005, in questa galassia, è stata individuata la supernova di tipo Ic. (it)
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| - MCG+07-33-027 (en)
- PGC56779 (en)
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| - Starburst galaxy MCG+07-33-027. (en)
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| - MCG+07-33-027 هي مجرة حلزونية منعزلة تقع على بعد 330 مليون سنة ضوئية في كوكبة الجاثي. تمتلك نسبة عالية جداً من تشكيل النجوم التي من شأنها أن تجعل من المجرة مجرة انفجار نجمي. عادةً، المجرات تنفجر بسبب اصطدام مجرة أخرى. ومع ذلك معظم المجرات هي في مجموعات أو تجمعات عنقودية، في حين أن مجرة MCG+07-33-027 انفرادية. لذلك، فإن سبب الإنفجار لم يكن بسبب الاصطدام أو بمرور مجرة مجاورة، وبالتالي فإن سبب النشاط لا يزال مجهولاً. (ar)
- MCG+07-33-027 is an isolated spiral galaxy located about 330 million light-years away in the constellation Hercules. It has a very high rate of star formation which would make it a starburst galaxy. Normally, starburst galaxies are triggered by the collision of another galaxy. However most galaxies are in groups or clusters, while MCG+07-33-027 is solitary. Therefore, the cause of the starburst was not due to a collision or by the passing of a nearby galaxy and so the cause of the activity remains unknown. On April 2, 2005, SN 2005bk, a supernova of type Ic was discovered in MCG+07-33-027. (en)
- MCG+07-33-027 è una galassia a spirale (S0) situata nella costellazione di Ercole alla distanza di oltre 330 milioni di anni luce dalla Terra. L'immagine raccolta dal Telescopio spaziale Hubble ci mostra la galassia vista di faccia (face-on). È una galassia starburst in cui è presente un'elevata attività di formazione stellare, ad un tasso di circa 100 nuovi astri all'anno. Ma dal momento che è una cosiddetta galassia di campo, cioè si trova in una posizione piuttosto isolata, l'intensa formazione di nuove stelle non può essere spiegata a causa di interazioni gravitazionali con altre galassie. Al momento non è stata formulata alcuna ipotesi plausibile. Nel 2005, in questa galassia, è stata individuata la supernova di tipo Ic. (it)
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