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IRAS 17449+2320: A Possible Binary System with the B[e] Phenomenon and a Strong Magnetic Field

We report the recent results of a long-term spectroscopic and photometric monitoring of IRAS 17449+2320, a member of the least studied group of objects with the B[e] phenomenon called FS CMa-type objects. The main hypothesis for explaining the strong emission-line spectra and infrared excesses of th...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: Sergey Zharikov, Anatoly Miroshnichenko, Inna Reva, Raushan Kokumbaeva, Chingis Omarov, Steve Danford, Alicia Aarnio, Nadine Manset, Ashish Raj, S. Drew Chojnowski, Joseph Daglen
Format: Artigo
Sprache:Inglês
Veröffentlicht: MDPI AG 2025-03-01
Schriftenreihe:Galaxies
Schlagworte:
early-type stars
emission line stars
magnetic fields
spectroscopy
photometry
Online-Zugang:https://www.mdpi.com/2075-4434/13/2/32
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