We present a multiwavelength analysis of a young bubble in the nuclear starburst of NGC 253 using new JWST MIRI–MRS observations together with archival ALMA (100, 350, 690 GHz) and Chandra data. The MIRI maps reveal a prominent bubble-like structure in both ionized and molecular emission lines. The bubble is spatially...
Kaitlyn E. Sheriff, E. Mills, Xin-Yu Mai et al.· Astronomical Journal· 0 citations
We present results from a spectroscopic survey of 32 FGK stars hosting brown dwarfs, using high-resolution optical spectra (R = 130,000 and 50,000) obtained with the Potsdam Echelle Polarimetric and Spectroscopic Instrument spectrograph on the Large Binocular Telescope. The primary goal of this survey is to determine p...
C. Phillips, Megan Bedell, Catherine Manea et al.· Astrophysical Journal· 0 citations
We present a structural, kinematic, and photometric analysis of the young, red supergiant- and Be star-rich open cluster NGC 7419 using Gaia DR3 and 2MASS data. This cluster is located at equatorial coordinates α= 343.58 ± 0.06◦and δ= 60.81 ± 0.03◦. By applying the HDBSCAN algorithm and adopting a conservative memb...
Nasser M. Ahmed, Remziye Canbay, D. Çınar· Research in Astronomy and As...· 0 citations
Open clusters are fundamental laboratories for investigating stellar and Galactic evolution, and serve as important benchmarks for asteroseismic analyses. Using a “boutique” method to analyze TESS photometry, we study red giants in two old supersolar-metallicity open clusters: NGC 188 and NGC 6791. By comparing Kepler...
Madeline Howell, Jennifer A. Johnson, M. Pinsonneault et al.· Astrophysical Journal· 0 citations
Classical Ae (CAe) stars are main-sequence, A-type stars with Hα emission but no signature of dust; they are thought to be the cool extension of classical Be (CBe) stars to lower stellar masses. We investigate the use of Hα and the Ca ii IR triplet observed at low spectroscopic resolution ( R=1800 ) as diagnostics for...
R. Anusha, T. A. A. Sigut· Astrophysical Journal· 0 citations
The Hubble constant (H0) quantifies the present-day expansion rate of the Universe and is a fundamental parameter for determining its age; however, modern cosmology faces significant tension, as increasingly precise measurements continue to yield mutually inconsistent values. The two main methods of measuring H0, namel...
Audrey Lee, T. Somboonpanyakul· Journal of emerging investig...· 0 citations
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