Tracing the Galactic Anticenter Stellar Stream with 2MASS M Giants

By H. Rocha-Pinto, S. Majewski, M. Skrutskie, J. Crane. 2003

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Citations in the corpus

Exploring Halo Substructure with Giant Stars. XI. The Tidal Tails of the Carina Dwarf Spheroidal Galaxy and the Discovery of Magellanic Cloud Stars in the Carina Foreground (2006, background): “…been made (including the one presented here in the foreground of Carina, see §6): the Monoceros/GASS stream (Newberg et al. 2002; Ibata et al. 2003; Rocha-Pinto et al. 2003; Crane et al. 2003), the TriAnd structure (Rocha-Pinto et al. 2004, Majewski et al. 2004), the M31 giant southern stream…”
A Two Micron All Sky Survey View of the Sagittarius Dwarf Galaxy. II. Swope Telescope Spectroscopy of M Giant Stars in the Dynamically Cold Sagittarius Tidal Stream (2004, background): “Interestingly, this is the general direction of the ‘‘ring’’ feature (Ibata et al. 2003; Yanny et al. 2003; Rocha-Pinto et al. 2003) identified with the potential ‘‘new galaxy’’ or tidal feature S223+20-19.4 by Newberg et al. (2002).”
Dark matter in the Milky Way II. The HI gas distribution as a tracer of the gravitational potential (2007, background): “The radiusR = 18.5 kpc of the dark matter ring in this direction implies that this object is located behind Canis Major and instead associated with “the One Ring” dis- cussed previously by Newberg et al. (2002); Ibata et al. (2003); Rocha-Pinto et al. (2003) and Yanny et al. (2003).”
The Milky Way Tomography with SDSS. I. Stellar Number Density Distribution (2005, background): “Examples include the Sgr dwarf tidal stream in the halo (Ivezić et al. 2000; Yanny et al. 2000; Vivas et al. 2001; Majewski et al. 2003) or the Monoceros stream closer to the Galactic plane (Newberg et al. 2002; Rocha-Pinto et al. 2003).”
Target Selection for the SDSS-IV APOGEE-2 Survey (2017, background): “…refinements to existing knowledge and new discoveries: for example, the properties of stellar substructure in the outskirts of the disk (with 2MASS; Rocha-Pinto et al. 2003), the existence of a long bar extending 2 kpc beyond the bulge (with GLIMPSE; Benjamin et al. 2005), variations in the IR…”
Outer structure of the Galactic warp and flare: explaining the Canis Major over-density (2006, background): “17 we show the location of positive Mon. Ring de- tections with respect to the warped and flared Milky Way disk.”
A New Milky Way Dwarf Galaxy in Ursa Major (2005, background): “…(Willman et al. 2005a) and a faint M31 dwarf satellite (Zucker et al. 2004), as well as large-scale stellar structures and dwarf galaxy remnants around the Milky Way (Newberg et al. 2002; Yanny et al. 2003; Ibata et al. 2003; Rocha-Pinto et al. 2003, 2004; Majewski et al. 2003; Martin et al. 2004).”
A Comprehensive Model for the Monoceros Tidal Stream (2004, background): “Tracing this structure with 2MASS M giant stars, Rocha-Pinto et al. (2003) concluded that its structural characteristics are consistent with the interpretation of this structure as the fossil of a merging dwarf galaxy, similar to the Sgr dwarf galaxy (Ibata et al. 1994), in the Galactic plane.”
RINGS AND RADIAL WAVES IN THE DISK OF THE MILKY WAY (2015, background): “In addition to structures that they identify as the Monoceros Ring (Ibata et al. 2003; though we argue below that this is not the Monoceros Ring), the TriAnd Stream (Rocha-Pinto et al. 2003), TriAnd2 (Martin et al. 2007), and the Pisces globular cluster stream (Bonaca et al. 2012; Martin et al. 2013”
A Two Micron All Sky Survey View of the Sagittarius Dwarf Galaxy. I. Morphology of the Sagittarius Core and Tidal Arms (2003, result): “Sloan find, and in two contributions (Rocha-Pinto et al. 2003; Crane et al. 2003) this 2MASS feature is explored further, with the conclusion that it is a new tidal tail system unrelated, but analogous, to that of the Sgr dwarf.”
Stellar Abundance and Galactic Chemical Evolution through LAMOST Spectroscopic Survey (2006, background): “Second, the spectacular discovery of debris from the Sagittarius dwarf galaxy shows a complete great circle throughout the sky (Rocha-Pinto et al. 2003).”
Chemodynamics of the Milky Way - I. The first year of APOGEE data (2013, methodology): “The development of sophisticated spectrophotometric parallax methods has been undertaken by many different groups in the past several years (e.g., Rocha-Pinto et al. 2003; Allende Prieto et al. 2006; Breddels et al. 2010; Zwitter et al. 2010; Burnett & Binney 2010; Burnett et al. 2011).”
The QUEST RR Lyrae Survey. II. The Halo Overdensities in the First Catalog (2006, background): “This stream appears to be part of a large ringlike structure that envelops the Milky Way (see also Majewski et al. 2003; Ibata et al. 2003; Rocha-Pinto et al. 2003; Peñarrubia et al. 2005; Conn et al. 2005a, 2005b).”