White Dwarfs Massive Stars Supernovae Star Formation Red Giants Planetary Nebulae Binary Stars Neutron Stars Red Supergiants Star Clusters White Dwarf Stars Star Life Cycle Star Explosions Binary Star Systems Dying Stars Protostars Supergiant Stars Star Types Young Stars Variable Stars Supernova Giant Stars Element Formation Black Hole Formation Planetary Science Star Composition Metal-Poor Stars Black Holes Brown Dwarfs Star Observation Star Classification Binary Systems Star Death Metallicity Star Systems Nucleosynthesis Sun Nuclear Fusion Population III Stars Planetary Formation Gravitational Perturbations Energy Production Models Star Mergers Massive Star Collapse Low Metallicity Stars Neutron Star Formation Main-Sequence Lifetimes Main-Sequence Stars Planetary Consumption Star-Planet Interactions Dwarf Stars Open Clusters Companion Stars Cataclysmic Variables End-of-Life Stars Sun-like Stars Supernova Mechanisms Stellar Structure Heavy Elements Low-Mass Stars Metal-free Stars Progenitor Stars Star-Forming Regions Star Interactions Cluster Dynamics Post-Main-Sequence Stars Planetary Systems Early Universe Stellar Death Life Cycle of Stars Planetary Nebula Nebulae Low-Intermediate Mass Stars Stellar Remnants Implications of Discovery Thermonuclear Explosions Pulsars Type Ia Supernovae Cepheid Variables Supergiants Exoplanets Magnetars Star Lifecycle Cosmic Events Stellar Mergers Hydrogen Burning Supernova Remnants Triple Star Systems Protoplanetary Disks Aging Stars Starquakes Star Collapse Wolf-Rayet Stars Supernovas Stellar Explosions Core Collapse Red Supergiant Stars Stellar Ages Star Explosion
The team will build a reference library of infrared fingerprints for astronomers.
