A peculiar Type II QSO identified via broad-band detection of extreme nebular line emission

Yu Heng Lin, Claudia Scarlata, Matthew Hayes, Anna Feltre, Stephane Charlot, Angela Bongiorno, Petri Väisänen, Moses Mogotsi

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

We present S82-20, an unusual redshift ≈3 object identified in SDSS-Stripe 82 broad-band images. The rest-frame ultraviolet spectrum of S82-20 shows emission lines from highly ionized species, including He ii 1640, and the C iv 1548, 1550 and O vi 1032, 1038 doublets. The high Ly α luminosity (3.5 × 1044 erg s-1), the high emission line equivalent widths (>200 Å for Ly α), the full width at half-maxim of the emission lines (<800 km s-1), and the high ionization O vi line strongly support the interpretation that S82-20 is a Type II Quasi-Stellar Objects (QSOs). However, photoionization models using Type II QSO do not fully explain the measured C iv/He ii line ratio, which requires either some contribution from star foation or high velocity shocks. Additionally, S82-20 is not detected at wavelengths longer than 2 in tension with the expectation of isotropically infrared emission of a luminous QSO. We consider the possibility that S82-20 is a rare example of a changing-look QSO, observed in a temporarily low state, where the broad line region has faded, while the narrow line region still emits emission line. Otherwise, it may be a rare case of the short phase of the life of a massive galaxy, in which active star foation and accretion on to a supeassive black hole coexist.

Original languageEnglish (US)
Pages (from-to)489-500
Number of pages12
JournalMonthly Notices of the Royal Astronomical Society
Volume509
Issue number1
DOIs
StatePublished - Jan 1 2022

Bibliographical note

Publisher Copyright:
© 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.

Keywords

  • active
  • emission lines
  • galaxies
  • high-redshift
  • quasars

Fingerprint

Dive into the research topics of 'A peculiar Type II QSO identified via broad-band detection of extreme nebular line emission'. Together they form a unique fingerprint.

Cite this