High velocity star?
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Or double supernova, or solar object? Wildly guessing is fun!
But seriously; how come the position of this 'star' is so far off in DECaLS in comparison to SDSS?
Does this fall within a standard timeframe for star position movement?http://skyserver.sdss.org/dr9/en/tools/explore/obj.asp?id=1237663542612459793
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Doesn't seem like an artifact looking at shape, and present in DECaLS and SDSS. But also not visible in earlier SDSS imaging, maybe obscured?
http://skyserver.sdss.org/dr5/en/tools/chart/navi.asp?ra=337.710463&dec=-0.524184
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by Budgieye moderator
Let me think... This green object seems to have moved 2 " (2 arc-seconds) in 10? years. (0.2 arc-sec/yr ?)
Hypervelocity star can move 0.19 arcsec/year , or 1.9 arcsec in 10 ish years.
So this object could be a hypervelocity star?
A fast moving neutron star? They are usually very blue, but magnetic white dwarfs are all sorts of funny colours.
or
Two unrecorded supernova, going off at different times? Green is the usual colour for a supernova in SDSS, and these are green.
4.1 Supernova in Talk, Forum, SDSS The Legacy Survey: Stripe 82, and Galaxy Zoo: The Hunt for Supernova. BBC Stargazing Live Snapshot Supernova http://talk.galaxyzoo.org/#/boards/BGZ0000001/discussions/DGZ0000wrb?page=4&comment_id=53d8b997db90c7673f00101d
Info on high velocity stars : white dwarf stars, neutron stars http://talk.galaxyzoo.org/#/boards/BGZ0000001/discussions/DGZ0000wrb?page=4&comment_id=53d8b9d1db90c76202001111
Forum thread: Hyper-Velocity Stars Project by Lovethetropics http://www.galaxyzooforum.org/index.php?topic=276167.0
Zooniverse Letters http://letters.zooniverse.org/ In-house publication of science results, Hypervelocity star project Zooites go off on a tangent with HVS by Love The Tropics 2012 "Abstract: A Hyper-Velocity Star is a star which has obtained galactic escape velocity. The existence of stars with this characteristic was first proposed in 1988. ..List of confirmed Hyper-Velocity Stars as of September 2009" in SDSS
Just for interest: A catalog of northern stars with annual proper motions larger than 0.15" (LSPM-NORTH catalog). http://simbad.u-strasbg.fr/simbad/sim-id?submit=display&bibdisplay=refsum&bibyear1=1983&bibyear2=2015&Ident=%404002025&Name=NLTT+19480#lab_bib
These are SIMBAD objects, and Ghost_Sheep_SWR's star is not a SIMBAD object, it is too dimProper Motions
Proper Motion is the apparent angular motion of a star across the sky with respect to more distant stars.* Typical proper motion is ~0.1 arcsec/year. * Largest: 10.25 arcsec/yr (Barnard's Star).
Hypervelocity star can move 0.19 arcsec/year
Note: proper motion in SDSS page has been multiplied by 100 , Why? I dunno. But you have to divide proper motion by 100 to get arc-sec/year.
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by Budgieye moderator
calculating date of SDSS dr9 photo, under PhotoObj click Field
mjd_u 5.2936148E4
mjd_g 5.29361496E4
mjd_r 5.29361463E4
mjd_i 5.29361471E4
mjd_z 5.29361488E4Get rid of exponent 52936.149
http://www.csgnetwork.com/julianmodifdateconv.htmldate of photo 10-24-2003
dr5 image 5.219725E4 52197.25 date of photo 10-15-2001
DECaLS images released in May 2015, so maybe taken in 2014.
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Supernova was my first thought, but then i saw the SDSS image and got confused, and no SN reference whatsoever
So 2 arcsec / 10-ish years would be within range of a hypervelocity star. But with a difference of +/- 2 years between the SDSS images it should also be visible on SDSS DR5 image at roughly the same position. In combination with the green color my best guess is 2 supernova, ill tag it just in case, although seems improbable within this timeframe.
EDIT reference image, cant find a date on this one, but recognised as star.
APOGEE image
Is it possible for a hypervelocity star to go supernova?
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by c_cld
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Form Decals browser (sources checked) we get for the "star"
Source RA,Dec = 337.7101, -0.5233
Source type: P
Mags: g=21.59, r=19.76, z=20.23
Brick: 3376m005, Objid: 2589
Number of exposures: g=4, r=4, z=4
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From SDSS DR9
1237663542612459793
we getSTAR 337.70948196,-0.52366619
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Querying SQL command: select
60*dbo.fDistanceArcMinEq(337.70948196,-0.52366619,337.7101, -0.5233)
yields 2.586 arcsec!
We don't know the date of DEcals images but it seems to me too far apart SDSS shot to imprint a much brighter persistence of an "hyperveloce" supernova.
That's why I am dubious about the SDSS "star" which could be a "muffin" from the nearby star mag. 9 (id=1237663542612525074), the second less possible interpretation is two different supernovae.
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Thank everyone for the information, i was confusing 2 different type of objects anyway.
And without further imaging or spectrum i don't think we can't get anymore certainty about this object or objects.
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