TY - JOUR
T1 - SAGITTARIUS II, DRACO II and LAEVENS 3
T2 - THREE NEW MILKY WAY SATELLITES DISCOVERED in the PAN-STARRS 1 3π SURVEY
AU - Laevens, Benjamin P.M.
AU - Martin, Nicolas F.
AU - Bernard, Edouard J.
AU - Schlafly, Edward F.
AU - Sesar, Branimir
AU - Rix, Hans Walter
AU - Bell, Eric F.
AU - Ferguson, Annette M.N.
AU - Slater, Colin T.
AU - Sweeney, William E.
AU - Wyse, Rosemary F.G.
AU - Huxor, Avon P.
AU - Burgett, William S.
AU - Chambers, Kenneth C.
AU - Draper, Peter W.
AU - Hodapp, Klaus A.
AU - Kaiser, Nicholas
AU - Magnier, Eugene A.
AU - Metcalfe, Nigel
AU - Tonry, John L.
AU - Wainscoat, Richard J.
AU - Waters, Christopher
PY - 2015/11/1
Y1 - 2015/11/1
N2 - We present the discovery of three new Milky Way satellites from our search for compact stellar overdensities in the photometric catalog of the Panoramic Survey Telescope and Rapid Response System 1 (Pan-STARRS 1, or PS1) 3π survey. The first satellite, Laevens 3, is located at a heliocentric distance of d = 67 � 3 kpc. With a total magnitude of MV = -4.4 � 0.3 and a half-light radius of rh = 7 � 2 pc, its properties resemble those of outer halo globular clusters. The second system, Draco II/Laevens 4, is a closer and fainter satellite (d ∼ 20 kpc, MV = -2.9 � 0.8), whose uncertain size (rh = 19-6 +8) renders its classification difficult without kinematic information; it could either be a faint and extended globular cluster or a faint and compact dwarf galaxy. The third satellite, Sagittarius II/Laevens 5 (Sgr II), has an ambiguous nature, as it is either the most compact dwarf galaxy or the most extended globular cluster in its luminosity range (rh = 37-8 +9 and MV = -5.2 � 0.4). At a heliocentric distance of 67 � 5 kpc, this satellite lies intriguingly close to the expected location of the trailing arm of the Sagittarius stellar stream behind the Sagittarius dwarf spheroidal galaxy (Sgr dSph). If confirmed through spectroscopic follow up, this connection would locate this part of the trailing arm of the Sagittarius stellar stream that has so far gone undetected. It would further suggest that Sgr II was brought into the Milky Way halo as a satellite of the Sgr dSph.
AB - We present the discovery of three new Milky Way satellites from our search for compact stellar overdensities in the photometric catalog of the Panoramic Survey Telescope and Rapid Response System 1 (Pan-STARRS 1, or PS1) 3π survey. The first satellite, Laevens 3, is located at a heliocentric distance of d = 67 � 3 kpc. With a total magnitude of MV = -4.4 � 0.3 and a half-light radius of rh = 7 � 2 pc, its properties resemble those of outer halo globular clusters. The second system, Draco II/Laevens 4, is a closer and fainter satellite (d ∼ 20 kpc, MV = -2.9 � 0.8), whose uncertain size (rh = 19-6 +8) renders its classification difficult without kinematic information; it could either be a faint and extended globular cluster or a faint and compact dwarf galaxy. The third satellite, Sagittarius II/Laevens 5 (Sgr II), has an ambiguous nature, as it is either the most compact dwarf galaxy or the most extended globular cluster in its luminosity range (rh = 37-8 +9 and MV = -5.2 � 0.4). At a heliocentric distance of 67 � 5 kpc, this satellite lies intriguingly close to the expected location of the trailing arm of the Sagittarius stellar stream behind the Sagittarius dwarf spheroidal galaxy (Sgr dSph). If confirmed through spectroscopic follow up, this connection would locate this part of the trailing arm of the Sagittarius stellar stream that has so far gone undetected. It would further suggest that Sgr II was brought into the Milky Way halo as a satellite of the Sgr dSph.
KW - galaxies: dwarf
KW - Galaxy: structure
KW - globular clusters: general
KW - Local Group
UR - http://www.scopus.com/inward/record.url?scp=84946734383&partnerID=8YFLogxK
U2 - 10.1088/0004-637X/813/1/44
DO - 10.1088/0004-637X/813/1/44
M3 - Article (Academic Journal)
AN - SCOPUS:84946734383
SN - 0004-637X
VL - 813
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
M1 - 44
ER -