Work

Optical spectroscopy of the IR source CPM 19 and surrounding objects

Year: 2026

Type: article

Source: Astrophysics

DOI: 10.1007/s10511-026-09963-9

Authors: T. Yu. Magakian, T. A. Movsessian, A. V. Moiseev, T. S. Molyarova, R. I. Uklein

Institutions: Byurakan Astrophysical Observatory, Special Astrophysical Observatory, University of Leeds

Language: English

Topic: Astrophysics and Star Formation Studies

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

Funders: National Science Foundation, Smithsonian Institution, National Aeronautics and Space Administration, Gordon and Betty Moore Foundation, Johns Hopkins University, Space Telescope Science Institute, Queen's University Belfast, Durham University, Queen's University, National Central University, Eötvös Loránd Tudományegyetem, Ministry of Science and Higher Education of the Russian Federation, Max-Planck-Institut für Astronomie, Smithsonian Astrophysical Observatory, Science Mission Directorate, Russian Academy of Sciences, Planetary Science Division, Los Alamos National Laboratory

Awards: G4474636675, G618131832, A NEO SEARCH PROGRAM USING THE PAN-STARRS PS1 TELESCOPETHE GOAL OF THE PROPOSED RESEARCH IS TO USE T, G7187964967, Pan-STARRS1: Operations; Public Data Release; Education and Outreach, G833430883

OpenAlex ID: W7140292535

FWCI:

Cites: 17

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