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20132017
most citedOn the distance of the Magellanic Clouds using Cepheid NIR and optical-NIR Period Wesenheit Relations

88 citations · 183 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201711 cited

Young and Intermediate-age Distance Indicators

Smitha Subramanian, Massimo Marengo, Anupam Bhardwaj +4

Distance measurements beyond geometrical and semi-geometrical methods, rely mainly on standard candles. As the name suggests, these objects have known luminosities by virtue of the…

astro-ph.GA201733 cited

Detailed chemical composition of classical Cepheids in the LMC cluster NGC 1866 and in the field of the SMC

B. Lemasle, M. A. T. Groenewegen, E. K. Grebel +11

Context: Cepheids are excellent tracers of young stellar populations. They play a crucial role in astrophysics as standard candles. The chemistry of classical Cepheids in the Milky…

astro-ph.GA2017

New classical Cepheids in the inner part of the northern Galactic disk and their kinematics

Satoshi Tanioka, Noriyuki Matsunaga, Kei Fukue +3

The characteristics of the inner Galaxy remain obscured by significant dust extinction, and hence infrared surveys are useful to find young Cepheids whose distances and ages can be…

astro-ph.GA201651 cited

A lack of classical Cepheids in the inner part of the Galactic disk

Noriyuki Matsunaga, Michael W. Feast, Giuseppe Bono +6

Recent large-scale infrared surveys have been revealing stellar populations in the inner Galaxy seen through strong interstellar extinction in the disk. In particular, classical Ce…

astro-ph.SR2013

On the relative distance of Magellanic Clouds using Cepheid NlR and Optical-NIR PW relations

L. Inno, G. Bono, N. Matsunaga +8

We present new estimates of the relative distance of the Magellanic Clouds (MCs) by using NIR and Optical-NIR Cepheid Period Wesenheit (PW) relations. The relative distances are in…

astro-ph.SR201388 cited

On the distance of the Magellanic Clouds using Cepheid NIR and optical-NIR Period Wesenheit Relations

L. Inno, N. Matsunaga, G. Bono +8

We present the largest near-infrared (NIR) data sets, , ever collected for classical Cepheids in the Magellanic Clouds (MCs). We selected fundamental (FU) and first overtone…