Blather split from Astronomer's Telegram: Supernova in M82
Posted: Wed Jan 22, 2014 4:30 pm
Oh wow, that's so interesting!!! :jumping up and down:
A red continuum, eh? Deep Na D absorption? A young, reddened Type Ia supernova? That sure makes sense. Without having seen a picture of the supernova (and hence knowing nothing about its location inside M82), I'm going to assume that the super-explosion took place fairly close to the region of rampant star formation near the galaxy's center. This region of star formation is extremely reddened from our point of view. Can you spot the young star clusters in this Hubble image of M82? All right, yes, you can spot some clusters in the disk, but it is very hard to see the clusters near the center of the galaxy, and that is because of the tremendous amounts of dust in this area.
M82 really is a very dusty galaxy. Its B (blue) magnitude is 9.161 ± 0.263, but its far infrared magnitude is 5.584 - about three and a half magnitudes brighter! This sort of "relationship" between the B and the far infrared magnitude can only mean that the galaxy is full of dust. Compare these values with the B and far infrared magnitudes of M82's neighbour, M81. The B magnitude of M81 is 7.849 ± 0.100. but its far infrared magnitude is 8.595. M81 is fainter in far infrared that in blue light and is likely quite poor in dust.
So, indeed, M82 is remarkably dusty. Therefore the supernova in M82 is most likely seen through a curtain of dust.
I can't help it, but I really like seeing that M82 has got a supernova that fits its host galaxy perfectly!!!
EDIT: Ah! Owlice has posted images of the supernova which show that the exploding star is not located close to the galaxy's center. Well, there is enough dust in M82 to go around, that much is certain.
Ann
A red continuum, eh? Deep Na D absorption? A young, reddened Type Ia supernova? That sure makes sense. Without having seen a picture of the supernova (and hence knowing nothing about its location inside M82), I'm going to assume that the super-explosion took place fairly close to the region of rampant star formation near the galaxy's center. This region of star formation is extremely reddened from our point of view. Can you spot the young star clusters in this Hubble image of M82? All right, yes, you can spot some clusters in the disk, but it is very hard to see the clusters near the center of the galaxy, and that is because of the tremendous amounts of dust in this area.
M82 really is a very dusty galaxy. Its B (blue) magnitude is 9.161 ± 0.263, but its far infrared magnitude is 5.584 - about three and a half magnitudes brighter! This sort of "relationship" between the B and the far infrared magnitude can only mean that the galaxy is full of dust. Compare these values with the B and far infrared magnitudes of M82's neighbour, M81. The B magnitude of M81 is 7.849 ± 0.100. but its far infrared magnitude is 8.595. M81 is fainter in far infrared that in blue light and is likely quite poor in dust.
So, indeed, M82 is remarkably dusty. Therefore the supernova in M82 is most likely seen through a curtain of dust.
I can't help it, but I really like seeing that M82 has got a supernova that fits its host galaxy perfectly!!!
EDIT: Ah! Owlice has posted images of the supernova which show that the exploding star is not located close to the galaxy's center. Well, there is enough dust in M82 to go around, that much is certain.
Ann