Context. Our view of the structure of the Milky Way and, in particular, its bulge is obscured by the intervening stars, dust, and gas in the disc. While great progress in understanding the bulge has been achieved with past and ongoing observations, the comparison of its global chemodynamical prop...
Gonzalez, O. A.
,
Gadotti, D. A.
,
Debattista, V. P.
,
Rejkuba, M.
,
Valenti, E.
,
Zoccali, M.
,
Coccato, L.
,
Minniti, D.
,
Ness, M.
,
[Comparing the properties of the X-shaped bulges of NGC 4710 and the Milky Way with MUSE]
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Comparing the properties of the X-shaped bulges of NGC 4710 and the Milky Way with MUSE
Context. Type II Cepheids (T2Cs) are radially pulsating variables that trace old stellar populations and provide distance estimates through their period-luminosity (PL) relation. Aims. We trace the structure of old stellar population in the Galactic bulge using new distance estimates and kinemati...
Braga, V.F.
,
Bhardwaj, A.
,
Contreras Ramos, R.
,
Minniti, D.
,
Bono, G.
,
De Grijs, R.
,
Minniti, J.H.
,
Rejkuba, M.
,
[Structure and kinematics of Type II Cepheids in the Galactic bulge based on near-infrared VVV data]
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Structure and kinematics of Type II Cepheids in the Galactic bulge based on near-infrared VVV data
We present the first stellar density profile of the Milky Way bulge that reaches latitude b = 0 degrees. The profile was derived by counting red clump stars within the colour-magnitude diagram that was constructed using the new PSF-fitting photometry from VISTA Variables in the Via Lactea (VVV) s...
Valenti, E.
,
Zoccali, M.
,
Gonzalez, O. A.
,
Minniti, D.
,
Alonso-García, J.
,
Marchetti, E.
,
Hempel, M.
,
Renzini, A.
,
Rejkuba, M.
,
[Stellar density profile and mass of the Milky Way bulge from VVV data]
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Stellar density profile and mass of the Milky Way bulge from VVV data