NAME Mercer 5 , the SIMBAD biblio

NAME Mercer 5 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.13CEST16:00:45


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Title First 3 Authors
2005ApJ...635..560M viz 15       D               92 126 New star clusters discovered in the GLIMPSE survey. MERCER E.P., CLEMENS D.P., MEADE M.R., et al.
2011A&A...532A.131B viz 38           X         1 108 104 New galactic star clusters discovered in the VVV survey. BORISSOVA J., BONATTO C., KURTEV R., et al.
2011MNRAS.416..465L 1882 T K A D S   X C F     46 33 12
Mercer 5: a probable new globular cluster in the Galactic bulge.
LONGMORE A.J., KURTEV R., LUCAS P.W., et al.
2011A&A...535A..33M 39         O X         1 20 49 Three galactic globular cluster candidates. MONI BIDIN C., MAURO F., GEISLER D., et al.
2012AJ....144..147O 39           X         1 16 7 Kronberger 49: a new low-mass globular cluster or an unprecedented bulge window? ORTOLANI S., BONATTO C., BICA E., et al.
2014MNRAS.437..843G 118           X C       2 28 21 IRC -10414: a bow-shock-producing red supergiant star. GVARAMADZE V.V., MENTEN K.M., KNIAZEV A.Y., et al.
2015A&A...575A..10D 40           X         1 69 12 First detections of FS Canis Majoris stars in clusters. Evolutionary state as constrained by coeval massive stars. DE LA FUENTE D., NAJARRO F., TROMBLEY C., et al.
2015PASP..127..329P 1191 T   A D     X C       29 21 3 Chemical abundances of the highly obscured Galactic globular clusters 2MASS GC02 and
Mercer 5.
PENALOZA F., PESSEV P., VASQUEZ S., et al.
2017ApJ...849L..24M 41           X         1 54 31 New VVV Survey globular cluster candidates in the Milky Way bulge. MINNITI D., GEISLER D., ALONSO-GARCIA J., et al.
2018MNRAS.476..690P 82             C       1 27 3 Chemical analysis of eight giant stars of the globular cluster NGC 6366. PULS A.A., ALVES-BRITO A., CAMPOS F., et al.
2018ApJ...863L..38R 41           X         1 40 13 Discovery of two new globular clusters in the Milky Way. RYU J. and LEE M.G.
2019MNRAS.482.5138B viz 185       D     X         5 167 293 Mean proper motions, space orbits, and velocity dispersion profiles of Galactic globular clusters derived from Gaia DR2 data. BAUMGARDT H., HILKER M., SOLLIMA A., et al.
2020MNRAS.491.3251P viz 230       D     X         6 83 44 Globular clusters in the inner Galaxy classified from dynamical orbital criteria. PEREZ-VILLEGAS A., BARBUY B., KERBER L.O., et al.
2020A&A...635A.125Y 17       D               1 149 ~ The origin of globular cluster FSR 1758. YEH F.-C., CARRARO G., KORCHAGIN V.I., et al.
2020MNRAS.495.1093H 834     A     X C       19 45 ~ Searches for pulsar-like candidates from unidentified objects in the Third Catalog of Hard Fermi-LAT Sources with machine learning techniques. HUI C.Y., LEE J., LI K.L., et al.
2021MNRAS.500.2937A 61       D     X         2 178 ~ The orbital evolution of UFDs and GCs in an evolving Galactic potential. ARMSTRONG B.M., BEKKI K. and LUDLOW A.D.
2021MNRAS.502.4547W 44           X         1 36 ~ The likelihood of undiscovered globular clusters in the outskirts of the Milky Way. WEBB J.J. and CARLBERG R.G.
2021MNRAS.505.5957B 104       D         F     2 165 126 Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST, and literature data. BAUMGARDT H. and VASILIEV E.
2021MNRAS.505.5978V viz 149       D     X         4 178 200 Gaia EDR3 view on galactic globular clusters. VASILIEV E. and BAUMGARDT H.
2023RAA....23a5013S 205       D     X         5 170 4 Classifying Globular Clusters and Applying them to Estimate the mass of the Milky Way. SUN G., WANG Y., LIU C., et al.
2023MNRAS.519.5059H 112       D         F     3 185 8 The accretion history of the Milky Way - I. How it shapes globular clusters and dwarf galaxies. HAMMER F., LI H., MAMON G.A., et al.
2023A&A...674A..70I 47           X         1 26 ~ Milky Way globular clusters on cosmological timescales II. Interaction with the Galactic centre. ISHCHENKO M., SOBOLENKO M., KUVATOVA D., et al.
2023A&A...678A..69I 47           X         1 35 ~ Milky Way globular clusters on cosmological timescales III. Interaction rates. ISHCHENKO M., SOBOLENKO M., BERCZIK P., et al.

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