Search Publications

Multiple Stellar Populations of Globular Clusters from Homogeneous Ca-CN-CH-NH Photometry. VI. M3 (NGC 5272) Is Not a Prototypical Normal Globular Cluster
DOI: 10.3847/1538-4357/abd948 Bibcode: 2021ApJ...909..167L

Sneden, Christopher; Lee, Jae-Woo

We present Ca-CN-CH-NH photometry for the well-known globular cluster (GC) M3 (NGC 5272). We show new evidence for two M3 populations with distinctly different carbon and nitrogen abundances, seen in a sharp division between CN-weak and CN-strong red-giant branches (RGBs) in M3. The CN-strong population shows a C-N anticorrelation that is a natura…

2021 The Astrophysical Journal
Gaia eHST 15
Magnetic Fields of CP Stars in the Orion OB1 Association. V. Stars of Subgroups (c) and (d)
DOI: 10.1134/S1990341321020085 Bibcode: 2021AstBu..76..163R

Romanyuk, I. I.; Semenko, E. A.; Moiseeva, A. V. +2 more

—The paper presents the results of magnetic field measurements of 27 chemically peculiar stars in subgroups (c) and (d) of the Orion OB1 association. In total, more than 140 circularly polarized spectra were obtained and measured in the period from 2013 to 2020. An analysis of the results showed that 13 out of 24 CP stars in subgroup (c) have a ma…

2021 Astrophysical Bulletin
Gaia 15
A MUSE spectro-imaging study of the Th 28 jet: Precession in the inner jet
DOI: 10.1051/0004-6361/202141315 Bibcode: 2021A&A...652A.119M

Ray, T. P.; Eislöffel, J.; Bacciotti, F. +5 more

Context. Th 28 is a Classical T Tauri star in the Lupus 3 cloud that drives an extended bipolar jet. Previous studies of the inner jet identified signatures of rotation around the outflow axis, a key result for theories of jet launching. Thus this is an important source in which to investigate the poorly understood jet launching mechanism.
Ai…

2021 Astronomy and Astrophysics
eHST 15
Probing Protoplanetary Disk Winds with C II Absorption
DOI: 10.3847/1538-4357/ac1739 Bibcode: 2021ApJ...921..181X

Herczeg, Gregory J.; France, Kevin; Johns-Krull, Christopher M. +1 more

We present an analysis of wind absorption in the C II λ1335 doublet toward 40 classical T Tauri stars with archival far-ultraviolet (FUV) spectra obtained by the Hubble Space Telescope. Absorption features produced by fast or slow winds are commonly detected (36 out of 40 targets) in our sample. The wind velocity of the fast wind decreases with di…

2021 The Astrophysical Journal
Gaia eHST 15
Toward Precise Galaxy Evolution: A Comparison between Spectral Indices of z 1 Galaxies in the IllustrisTNG Simulation and the LEGA-C Survey
DOI: 10.3847/1538-3881/ac20d6 Bibcode: 2021AJ....162..201W

Bell, Eric F.; Maseda, Michael V.; Muzzin, Adam +13 more

We present the first comparison of observed stellar continuum spectra of high-redshift galaxies and mock galaxy spectra generated from hydrodynamical simulations. The mock spectra are produced from the IllustrisTNG TNG100 simulation combined with stellar population models and take into account dust attenuation and realistic observational effects (…

2021 The Astronomical Journal
eHST 15
Observing and modelling the young solar analogue EK Draconis: starspot distribution, elemental abundances, and evolutionary status
DOI: 10.1093/mnras/stab199 Bibcode: 2021MNRAS.502.3343S

Solanki, S. K.; Montes, D.; Hussain, G. A. J. +4 more

Observations and modelling of stars with near-solar masses in their early phases of evolution are critical for a better understanding of how dynamos of solar-type stars evolve. We examine the chemical composition and the spot distribution of the pre-main-sequence solar analogue EK Dra. Using spectra from the HERMES Spectrograph (La Palma), we obta…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 15
Modeling of Possible Plume Mechanisms on Europa
DOI: 10.1029/2021JA029690 Bibcode: 2021JGRA..12629690V

Wurz, Peter; Vorburger, Audrey

Plumes spewing water high above Europa's surface have been inferred from several observation campaigns in the past decade. Whereas the occasional existence of plumes on Europa has thus been confirmed, the origin of the plumes remains uncertain. Most notably, it is still unclear whether the inferred plumes are of oceanic origin, possibly containing…

2021 Journal of Geophysical Research (Space Physics)
eHST 15
Convection and rotation boosted prescription of magnetic braking: application to the formation of extremely low-mass white dwarfs
DOI: 10.1093/mnras/stab1916 Bibcode: 2021MNRAS.506.3266S

Kepler, S. O.; Soethe, L. T. T.

Extremely low-mass white dwarfs (ELM WDs) are the result of binary evolution in which a low-mass donor star is stripped by its companion leaving behind a helium-core white dwarf (WD). We explore the formation of ELM WDs in binary systems considering the Convection And Rotation Boosted magnetic braking treatment. Our evolutionary sequences were cal…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 15
A Deep Polarimetric Study of the Asymmetrical Debris Disk HD 106906
DOI: 10.3847/1538-4357/abff5c Bibcode: 2021ApJ...915...58C

MacGregor, Meredith A.; Weinberger, Alycia J.; Debes, John H. +16 more

Located in the Lower Centaurus Crux group, HD 106906 is a young, binary stellar system. This system is unique among discovered systems in that it contains an asymmetrical debris disk, as well as an 11 MJup planet companion, at a separation of ~735 au. Only a handful of other systems are known to contain both a disk and a directly imaged…

2021 The Astrophysical Journal
Gaia 15
Toward the true number of flaring giant stars in the Kepler field. Are their flaring specialities associated with their being giant stars?
DOI: 10.1051/0004-6361/202039674 Bibcode: 2021A&A...647A..62O

Pál, A.; Günther, M. N.; Oláh, K. +4 more


Aims: We aim to give a reliable estimate of the number of flaring giant stars in the Kepler field. By analyzing the flaring activity of these stars, we explored their flare statistics and the released flare energies. The role of oscillation in suppressing magnetic activity was also investigated. We searched for flaring specialities that may b…

2021 Astronomy and Astrophysics
Gaia 15