by Ann » Sun Aug 04, 2019 12:01 pm
Wide-angle view of lenticular galaxy NGC 4526.
Note that the conspicuous star to the right of the dusty disk is not the supernova.
Credit:ESA/Hubble & NASA, Acknowledgement: Judy Schmidt
I presume that the supernova is the star at 7 o'clock in the APOD?
JOhn
Yes.
"In the outskirts of a galaxy"? That nova is half a galactic radius outside the rim! It's not in the outskirts, it's way, way beyond, so far as to question its association.
Like you said, the supernova is not not on the outskirts of NGC 4526, but that's because it was located about halfway between the core and the outer diffuse edge of the galaxy. The dusty disk in the APOD is just the small inner disk of the galaxy. Look at the picture at left!
Various online authorities give their distances from us as 55 and 50 million light years. Can't find a diameter for that galaxy, but they are quoted in thousands on LYs, and this star is 5 MIllion LY nearer to us?
Establishing exact distances of objects millions of light-years away is tricky. So an estimate of 50 to 55 million light-years for the galaxy and the supernova is good enough. But I'd say it is certain that the supernova and the galaxy are not 5 million light-years away from one another!
Light curves of 22 Supernovae type Ia. Source: ned.ipac.caltech.edu
Is the supernova really a part of NGC 4526?
Yes, absolutely!
The reasons why we can be so sure that Supernova 1994D really belonged to galaxy NGC 4526 are twofold. First, the supernova happened well inside this galaxy, about halfway between the center and the edge. Second, it was a type Ia supernova, and this type of supernovas have extremely distinctive light curves and well understood absolute luminosities. SN 1994D had just the sort of luminosity that could be expected from a supernova type Ia at the distance of NGC 4526.
Moreover, the fact that SN 1994D was a type Ia supernova means that it didn't receive a huge kick when it exploded, because SN type Ia don't function like that. The supernova remnants that can get a kick away from their birthplaces are core collapse supernovas, the ones that form neutron stars or black holes when they explode. Core collapse supernovas can explode asymmetrically and send their neutron stars or black holes flying.
So Supernova 1994 was not an interstellar visitor, and itself and its progenitor always belonged to galaxy NGC 4526.
Ann
[float=left][img2]https://cdn.spacetelescope.org/archives/images/screen/potw1442a.jpg[/img2][c][size=85][color=#0040FF]Wide-angle view of lenticular galaxy NGC 4526.
Note that the conspicuous star to the right of the dusty disk is not the supernova.
Credit:ESA/Hubble & NASA, Acknowledgement: Judy Schmidt[/color][/size][/c][/float]
[quote][b][color=#0040FF]I presume that the supernova is the star at 7 o'clock in the APOD[/color][/b]?
JOhn
[/quote]
Yes.
[quote]"In the outskirts of a galaxy"? That nova is half a galactic radius outside the rim! It's not in the outskirts, it's way, way beyond, so far as to question its association.
[/quote]
Like you said, the supernova is not not on the outskirts of NGC 4526, but that's because it was located about halfway between the core and the outer diffuse edge of the galaxy. The dusty disk in the APOD is just the small inner disk of the galaxy. Look at the picture at left!
[quote]Various online authorities give their distances from us as 55 and 50 million light years. Can't find a diameter for that galaxy, but they are quoted in thousands on LYs, and this star is 5 MIllion LY nearer to us? [/quote]
Establishing exact distances of objects millions of light-years away is tricky. So an estimate of 50 to 55 million light-years for the galaxy and the supernova is good enough. But I'd say it is certain that the supernova and the galaxy are not 5 million light-years away from one another!
[quote]Is it really part of NGC4526?
Could it be an intergalactic, 'rogue' star, ejected from another galaxy, as suggested by Ryan Foley? See: https://academic.oup.com/mnras/article/452/3/2463/1751818?sid=70ce50c3-f92e-46fe-977e-83b3af63f3d9
[/quote]
[float=left][img2]https://ned.ipac.caltech.edu/level5/Branch2/Figures/figure2.jpeg[/img2][c][size=85][color=#0040FF]Light curves of 22 Supernovae type Ia. Source: ned.ipac.caltech.edu[/color][/size][/c][/float]Is the supernova really a part of NGC 4526? [b][color=#FF40FF]Yes, absolutely[/color][/b]!
The reasons why we can be so sure that Supernova 1994D really belonged to galaxy NGC 4526 are twofold. First, the supernova happened well inside this galaxy, about halfway between the center and the edge. Second, it was a type Ia supernova, and this type of supernovas have extremely distinctive light curves and well understood absolute luminosities. SN 1994D had just the sort of luminosity that could be expected from a supernova type Ia at the distance of NGC 4526.
Moreover, the fact that SN 1994D was a type Ia supernova means that it didn't receive a huge kick when it exploded, because SN type Ia don't function like that. The supernova remnants that can get a kick away from their birthplaces are core collapse supernovas, the ones that form neutron stars or black holes when they explode. Core collapse supernovas can explode asymmetrically and send their neutron stars or black holes flying.
So Supernova 1994 was not an interstellar visitor, and itself and its progenitor always belonged to galaxy NGC 4526.
Ann