Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event

التفاصيل البيبلوغرافية
العنوان: Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event
المؤلفون: Zang, Weicheng, Dong, Subo, Gould, Andrew, Novati, Sebastiano Calchi, Chen, Ping, Yang, Hongjing, Li, Shun-Sheng, Mao, Shude, Alton, K. B., Carey, Sean, Christie, G. W., Delplancke-Ströbele, F., Feliz, Dax L., Green, J., Hu, Shaoming, Jayasinghe, T., Koff, R. A., Kurtenkov, A., Mérand, A., Minev, Milen, Mutel, Robert, Natusch, T., Roth, Tyler, Shvartzvald, Yossi, Sun, Fengwu, Vanmunster, T., Zhu, Wei
سنة النشر: 2019
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics
الوصف: We report the lens mass and distance measurements of the nearby microlensing event TCP J05074264+2447555. We measure the microlens parallax vector ${\pi}_{\rm E}$ using Spitzer and ground-based light curves with constraints on the direction of lens-source relative proper motion derived from Very Large Telescope Interferometer (VLTI) GRAVITY observations. Combining this ${\pi}_{\rm E}$ determination with the angular Einstein radius $\theta_{\rm E}$ measured by VLTI GRAVITY observations, we find that the lens is a star with mass $M_{\rm L} = 0.495 \pm 0.063~M_{\odot}$ at a distance $D_{\rm L} = 429 \pm 21~{\rm pc}$. We find that the blended light basically all comes from the lens. The lens-source proper motion is $\mu_{\rm rel,hel} = 26.55 \pm 0.36~{\rm mas\,yr^{-1}}$, so with currently available adaptive-optics (AO) instruments, the lens and source can be resolved in 2021. This is the first microlensing event whose lens mass is unambiguously measured by interferometry + satellite parallax observations, which opens a new window for mass measurements of isolated objects such as stellar-mass black holes.
Comment: 3 Figures and 6 Tables Submitted to AAS Journal
نوع الوثيقة: Working Paper
DOI: 10.3847/1538-4357/ab9749
URL الوصول: http://arxiv.org/abs/1912.00038
رقم الأكسشن: edsarx.1912.00038
قاعدة البيانات: arXiv
الوصف
DOI:10.3847/1538-4357/ab9749