SIMBAD references

2023ApJ...953...86C - Astrophys. J., 953, 86 (2023/August-2)

Modeling the Multiwavelength Evolution of the V960 Mon System.

CARVALHO A.S., HILLENBRAND L.A., HAMBSCH F.-J., DVORAK S., SITKO M., RUSSELL R.W., HAMMOND V., CONNELLEY M., ASHLEY M.C.B. and HANKINS M.J.

Abstract (from CDS):

We study the evolution of the FU Ori object V960 Mon since its outburst, using available multiwavelength photometric time series over 8 yr, complemented by several epochs of moderate-dispersion spectrophotometry. We find that the source fading can be well-described by a decrease in the temperature of the inner disk, which results from a combination of decreasing accretion rate and increasing inner disk radius. We model the system with a disk atmosphere model that produces the observed variations in multiband photometry (this paper) and high-resolution spectral lines (a companion paper).

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): FU Orionis stars - Young stellar objects - Infrared sources - Stellar accretion disks - Optical bursts

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 3

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