Astrometry of H2O Masers in Nearby Star-Forming Regions with VERA II SVS 13 in NGC 1333

By T. Hirota, T. Bushimata, Y. Choi, M. Honma, H. Imai, K. Iwadate, T. Jike, O. Kameya, R. Kamohara, Y. Kan-ya and 18 more. 2008

138 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/faedbbbd44e4dbedae52ea1821059f83b7d43ad9

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In Astronomy and Astrophysics

Citations in the corpus

THE WISE CATALOG OF GALACTIC H ii REGIONS (2013, background): “…et al. 2008; (7) Brunthaler et al. 2009; (8) Caswell & Haynes 1987; (9) Dunham et al. 2011; (10) Hachisuka et al. 2009; (11) Hirota et al. 2008a; (12) Hirota et al. 2008c; (13) Honma et al. 2007; (14) Honma et al. 2011; (15) Immer et al. 2013; (16) Jones & Dickey 2012; (17) Kurayama et al. 2011;…”
THE VLA NASCENT DISK AND MULTIPLICITY SURVEY OF PERSEUS PROTOSTARS (VANDAM). II. MULTIPLICITY OF PROTOSTARS IN THE PERSEUS MOLECULAR CLOUD (2016, background): “Most, however, were found with separations >400 au (corrected for the updated distance to Perseus, d∼230 pc Hirota et al. 2008, 2011).”
Kinematics in Young Star Clusters and Associations with Gaia DR2 (2018, methodology): “In Appendix A we compare our distance estimate to 386±8 pc from Kounkel et al. (2018) and discuss effects of the three-dimensional structure of Orion A. • Our distance estimate for NGC 1333 of 296±5 pc is ∼25% larger than the distance from Hirota et al. (2008) of 235±18 pc.”
Microarcsecond Radio Astrometry (2013, background): “Observing H2O masers, Hirota et al. (2008) measured parallax distances of 235 ± 18 pc for the SVS 13 toward NGC 1333 and 232 ± 18 pc for L 1448 C (Hirota et al. 2011).”
TADPOL: A 1.3 mm SURVEY OF DUST POLARIZATION IN STAR-FORMING CORES AND REGIONS (2013, background): “Using VLBI observations of 22GHz H2O masers, Hirota et al. (2008) found a distance of 235 pc. Observations at millimeter wavelengths reveal at least three continuum sources within SVS 13.”
A LARGE CATALOG OF ACCURATE DISTANCES TO MOLECULAR CLOUDS FROM PS1 PHOTOMETRY (2014, background): “Literature estimates of the cloud distance range from 350 pc (Herbig & Jones 1983) to parallax estimates of about 230 pc from Hirota et al. (2008) and Hirota et al. (2011).”
Milky Way mass models for orbit calculations (2012, background): “…this argument, parallaxes, proper motions, and heliocentric radial velocities for 30 maser sources have been compiled from the literature (Sandstrom et al. 2007; Hirota et al. 2008a,b; Reid et al. 2009; Rygl et al. 2010; Sato et al. 2010; Asaki et al. 2010; Niinuma et al. 2011; Honma et al. 2011).”