Spoon-Feeding Giant Stars to Supermassive Black Holes: Episodic Mass Transfer from Evolving Stars and Their Contribution to the Quiescent Activity of Galactic Nuclei

TL;DR

This paper investigates a gradual, episodic mass transfer process from evolving giant stars to supermassive black holes, which may significantly contribute to the low-level activity of galactic nuclei.

Contribution

It introduces the concept of spoon-feeding giant stars through episodic mass transfer as a new mechanism for SMBH fueling, differing from traditional tidal disruption events.

Findings

Giant stars can transfer mass to SMBHs over many orbits, creating recurrent low-level flares.

This feeding mode is significant for SMBHs over 10 million solar masses.

Spoon-feeding may influence the quiescent luminosity of SMBHs.

Abstract

Stars may be tidally disrupted if, in a single orbit, they are scattered too close to a supermassive black hole (SMBH). Tidal disruption events are thought to power luminous but short-lived accretion episodes that can light up otherwise quiescent SMBHs in transient flares. Here we explore a more gradual process of tidal stripping where stars approach the tidal disruption radius by stellar evolution while in an eccentric orbit. After the onset of mass transfer, these stars episodically transfer mass to the SMBH every pericenter passage giving rise to low-level flares that repeat on the orbital timescale. Giant stars, in particular, will exhibit a runaway response to mass loss and "spoon-feed" material to the black hole for tens to hundreds of orbital periods. In contrast to full tidal disruption events, the duty cycle of this feeding mode is of order unity for black holes with mass greater than approximately 10 million solar masses. This mode of quasi-steady SMBH feeding is competitive with indirect SMBH feeding through stellar winds, and spoon-fed giant stars may play a significant role in determining the quiescent luminosity of local SMBHs.