activity
20012009
most citedA Survey of Local Group Galaxies Currently Forming Stars. I. UBVRI Photometry of Stars in M31 and M33

412 citations · 1.5k across the 14 of their papers we have counts for

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astro-ph200891 cited

The Physical Properties and Effective Temperature Scale of O-type Stars as a Function of Metallicity. III. More Results from the Magellanic Clouds

Philip Massey, Amanda M. Zangari, Nidia I. Morrell +4

In order to better determine the physical properties of hot, massive stars as a function of metallicity, we obtained very high SNR optical spectra of 26 O and early B stars in the…

astro-ph200893 cited

The Massive Star Content of NGC 3603

Nicholas W. Melena, Philip Massey, Nidia I. Morrell +1

We investigate the massive star content of NGC 3603, the closest known giant H II region. We have obtained spectra of 26 stars in the central cluster using the Baade 6.5-m telescop…

astro-ph20086 cited

The Physical Properties of Red Supergiants: Comparing Theory and Observations

Philip Massey, Emily M. Levesque, Bertrand Plez +1

Red supergiants (RSGs) are an evolved stage in the life of intermediate massive stars (than than 25 solar masses). For many years, their location in the H-R diagram was at variance…

astro-ph2007176 cited

A Survey of Local Group Galaxies Currently Forming Stars: III. A Search for Luminous Blue Variables and Other H-alpha Emission-Lined Stars

Philip Massey, Reagin T. McNill, K. A. G. Olsen +5

We describe a search for H-alpha emission-lined stars in M31, M33, and seven dwarfs in or near the Local Group (IC 10, NGC 6822, WLM, Sextans B, Sextans A, Pegasus and the Phoenix…

astro-ph2007

The Coolest Stars in the Clouds: Unusual Red Supergiants in the Magellanic Clouds

Emily M. Levesque, Philip Massey, K. A. G. Olsen +1

Red supergiants (RSGs) are a He-burning phase in the evolution of moderately high mass stars (10-25 solar masses). The evolution of these stars, particularly at low metallicities,…

astro-ph200636 cited

Bringing VY Canis Majoris Down to Size: An Improved Determination of Its Effective Tempeature

Philip Massey, Emily M. Levesque, Bertrand Plez

The star VY CMa is a late-type M supergiant with many peculiarities, mostly related to the intense circumstellar environment due to the star's high mass-loss rate. Claims have been…