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

被引:8
作者
Chang, Seo-Won [1 ,2 ,3 ]
Wolf, Christian [4 ,5 ]
Onken, Christopher A. [4 ]
Bessell, Michael S. [4 ]
机构
[1] Seoul Natl Univ SNU, SNU Astron Res Ctr, 1 Gwanak Rho, Seoul 08826, South Korea
[2] SNU, Astron Program, Dept Phys & Astron, 1 Gwanak Rho, Seoul 08826, South Korea
[3] SNU, Ctr Gravitat Wave Universe, 1 Gwanak Rho, Seoul 08826, South Korea
[4] Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
[5] Australian Natl Univ, Ctr Gravitat Astrophys CGA, Acton, ACT 2601, Australia
基金
澳大利亚研究理事会; 新加坡国家研究基金会;
关键词
stars: fundamental parameters; stars: individual: SMSS J184506.82-300804.7; stars: oscillations; stars: variable: general; HOT SUBDWARF STARS; GAIA DR2; SURVIVING COMPANIONS; EVOLUTIONARY STATUS; B STARS; LIBRARY; DISK; II;
D O I
10.1093/mnras/stae637
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 similar to 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 T-eff = 29 020-34+193 K, logg = 4.661-0.143+0.008 (cm s(-2)), and logn(He)/n(H) = -2.722-0.074+0.057 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 similar to-2.4.
引用
收藏
页码:1414 / 1422
页数:9
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