activity
19972003
collaborators

5 papers

astro-ph2003

Near-Infrared Spectroscopy and Young Stellar Populations

Michael R. Meyer

Over the past decade, tremendous progress has been made in applying the techniques of MK classification to spectra obtained from 1-5 microns. This spectral region is rich in atomic…

astro-ph2002

Beyond the Cosmic Veil: Star and Planet Formation Research after SIRTF and NGST

Michael R. Meyer

How do planets form from circumstellar disks of gas and dust? What physical processes are responsible for determining the final masses of forming stars and ultimately the initial m…

astro-ph2002

Evolution of Brown Dwarf Atmospheres: Investigating Physical Parameters from Near-IR Spectra

Nadya Gorlova, Michael R. Meyer, Jim Liebert +1

We obtained near-infrared spectra of a sample of very low mass objects as a function of age in order to investigate the temperature and surface gravity sensitivity of several featu…

astro-ph1999

The Stellar Initial Mass Function: Constraints from Young Clusters and Theoretical Perspectives

Michael R. Meyer, Fred C. Adams, Lynne A. Hillenbrand +2

We summarize recent observational and theoretical progress aimed at understanding the origin of the stellar initial mass function (IMF) with specific focus on galactic star-forming…

astro-ph1997

Circumstellar Disks Around Pre-Main-Sequence Stars: What ISO Can Tell Us

A. Natta, M. R. Meyer, S. V. W. Beckwith

ISO observations will improve our understanding of disks around low-mass pre-main-sequence stars in various ways. In particular, ISO can measure simultaneously spectral energy dist…