Arp273 is actually a group of interacting galaxies with a
projected nuclear
separation of 40 kpc or 1.3x104 light years. 1. The two galaxies that make up Arp 273
are
known
independently as UGC01810 and UGC01813. UGC01810 is
the
larger more face on spiral galaxy and UGC01813 is the one that looks in
this image to be smaller and flatter (it is in fact a spiral like
UGC01810).
RA:2h21m28.700s
Classification: SA(s)b pec
Apparent Total Magnitude (B): 13.5 +/-less than .3mag 4
Colour: B-V= 0.047 mag 5
Red shift: 0.02523 +/-0.00004 6
Distance: Between 7.569 & 15.138 Mpc
* which is
equivalent to it being between 24.69 and
49.38 million light years away.++
Heliocentric radial velocity: 7563 +/-11 km/s 5
Group association: Part of the Percius Cluster7
RA: 2h18m27.536s
Apparent Total Magnitude (B): 15.2+/-less than 0.3mag4
Colour: B-V= 0.68 mag 5
Red shift: 0.02447 +/-0.00015 6
Distance: Between 7.341 & 14.682 Mpc
* which is
equivalent to it being between 23.946 and
47.893 million light years away.++
Heliocentric radial velocity: 7335 +/-46 km/s
Group association: Part of the Percius Cluster
7
* distance=0.01zc/h
Note: All references taken from NED unless otherwise indicated
UGC01810:
Dec:+39deg22'31.90"
Epoch:J2000 2

Diameters:
Bluesize
(POSS blue print)2.1x1.4 arcmin
3
Red size
(POSS red print)1.9x1.3 arcmin
3
UGC01813:
Dec: +39deg21'24.60"
Epoch: J2000 2

Classification: SB(s)a pec
Diameters:
Bluesize
(POSS blue print)1.4x0.4 arcmin
3
Red size
(POSS red print)1.4x0.4 arcmin
3
z is the redshift, c is the speed
of light & h represents the hubble
constant and is known to be between 0.5 & 1.0
++ 1 parsec=3.262 light years
(http://www.astro.virginia.edu/~jh8h/glossary/parsec.htm)
found
at:
http://leda.univ-lyon1.fr/cgi-bin/querybyname.pl?donnee=mean&objname=PGC+%2B008961
http://nedwww.ipac.caltech.edu/cgi-bin/nph-ex_refcode?refcode=1981ApJ...243..411G