Discovery of a new blue large-amplitude pulsator in the SkyMapper DR2: SMSS J184506.82−300804.7

Author:

Chang Seo-Won123ORCID,Wolf Christian45ORCID,Onken Christopher A4ORCID,Bessell Michael S4ORCID

Affiliation:

1. SNU Astronomy Research Center, Seoul National University (SNU) , 1 Gwanak-rho, Gwanak-gu, Seoul 08826 , Korea

2. Astronomy Program, Department of Physics & Astronomy, SNU , 1 Gwanak-rho, Gwanak-gu, Seoul 08826 , Korea

3. Center for the Gravitational-Wave Universe, SNU , 1 Gwanak-rho, Gwanak-gu, Seoul 08826 , Korea

4. Research School of Astronomy and Astrophysics, Australian National University , Weston Creek ACT 2611 , Australia

5. Centre for Gravitational Astrophysics (CGA), Australian National University , Acton ACT 2601 , Australia

Abstract

ABSTRACT We report the discovery of a new Blue Large-Amplitude Pulsator (BLAP), SMSS J184506−300804 (SMSS-BLAP-1) in Data Release 2 of the SkyMapper Southern Sky Survey. We conduct high-cadence photometric observations in the u band to confirm a periodic modulation of the light curve. SMSS-BLAP-1 has a ∼19-min pulsation period with an amplitude of 0.2 mag in u band, and is similar to the classical BLAPs found by OGLE. From spectroscopic observations with the Wide-Field Spectrograph on the Australian National University 2.3m telescope, we confirm it as a low-gravity BLAP: best-fitting parameters from the non-LTE tlusty model are estimated as Teff = 29 020$^{+193}_{-34}$ K, logg = 4.661$^{+0.008}_{-0.143}$ (cm s−2), and logn(He)/n(H) = −2.722$^{+0.057}_{-0.074}$ dex. However, our BLAP exhibits a very He-deficient atmosphere compared to both low- and high-gravity BLAPs, which have logn(He)/n(H) in the range −0.41∼−2.4.

Funder

National Research Foundation of Korea

MSIT

NRF

Ministry of Education

Australian Research Council

Publisher

Oxford University Press (OUP)

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