Search Publications

APOGEE-2S Discovery of Light- and Heavy-element Abundance Correlations in the Bulge Globular Cluster NGC 6380
DOI: 10.3847/2041-8213/ac1c7e Bibcode: 2021ApJ...918L...9F

Cunha, Katia; Smith, Verne V.; Majewski, Steven R. +11 more

We derive abundance ratios for nine stars in the relatively high-metallicity bulge globular cluster NGC 6380. We find a mean cluster metallicity between [Fe/H] = -0.80 and -0.73, with no clear evidence for a variation in iron abundances beyond the observational errors. Stars with strongly enhanced [N/Fe] abundance ratios populate the cluster and a…

2021 The Astrophysical Journal
Gaia 11
Mrk 1239: a Type-2 Counterpart of Narrow-line Seyfert-1?
DOI: 10.3847/1538-4357/abf148 Bibcode: 2021ApJ...912..118P

Zhou, Hongyan; Ji, Tuo; Shi, Xiheng +10 more

We present new spectrophotometric and spectropolarimetric observations of Mrk 1239, one of the 8 prototypes that defines type-1 narrow-line Seyfert galaxies (NLS1s). Unlike the other typical NLS1s though, a high degree of polarization (P ∼ 5.6%) and red optical-IR (g-W4 = 12.35) colors suggest that Mrk 1239 is more similar to type-2 act…

2021 The Astrophysical Journal
IUE eHST 11
Detecting Reconnection Sites Using the Lorentz Transformations for Electromagnetic Fields
DOI: 10.3847/1538-4357/abeb74 Bibcode: 2021ApJ...911..147L

Lapenta, Giovanni

We take a pragmatic definition of reconnection to find locations where a reconnection electric field causes an E × B drift that carries two components of the magnetic field toward their elimination. With this in mind as our target, we observe that such locations can be found using a new indicator: the velocity of the Lorentz transformation that el…

2021 The Astrophysical Journal
Cluster 11
Near-infrared Studies of Nova V1674 Herculis: A Shocking Record Breaker
DOI: 10.3847/2041-8213/ac3518 Bibcode: 2021ApJ...922L..10W

Banerjee, D. P. K.; Starrfield, S.; Page, K. L. +3 more

We present near-infrared spectroscopy of Nova Herculis 2021 (V1674 Her), obtained over the first 70 days of its evolution. This fastest nova on record displays a rich emission line spectrum, including strong coronal line emission with complex structures. The hydrogen line fluxes, combined with a distance of ${4.7}_{-1.0}^{+1.3}$ kpc, give an upper…

2021 The Astrophysical Journal
Gaia 11
14 Her: A Likely Case of Planet-Planet Scattering
DOI: 10.3847/2041-8213/ac382c Bibcode: 2021ApJ...922L..43B

Gelino, Christopher R.; Faherty, Jacqueline K.; Bardalez Gagliuffi, Daniella C. +4 more

In this Letter, we measure the full orbital architecture of the two-planet system around the nearby K0 dwarf 14 Herculis. 14 Her (HD 145675, HIP 79248) is a middle-aged ( ${4.6}_{-1.3}^{+3.8}$ Gyr) K0 star with two eccentric giant planets identified in the literature from radial velocity (RV) variability and long-term trends. Using archival RV dat…

2021 The Astrophysical Journal
Gaia Hipparcos 11
Sublimation of Laboratory Ices Millimeter/Submillimeter Experiment (SubLIME): Structure-specific Identifications of Products from UV-photolyzed Methanol Ice
DOI: 10.3847/1538-4357/abf14e Bibcode: 2021ApJ...913...61Y

Gerakines, P. A.; Milam, S. N.; Widicus Weaver, S. L. +1 more

Submillimeter/far-IR spectroscopy was used to detect and quantify organic molecules sublimated after the ultraviolet photolysis (at 12 K) and warm-up (up to 300 K) of a methanol (CH3OH) ice sample. Eleven sublimated photoproducts were uniquely identified: carbon monoxide (CO), formaldehyde (H2CO), ketene (C2H2…

2021 The Astrophysical Journal
Herschel Rosetta 11
HO Puppis: Not a Be Star, but a Newly Confirmed IW And-type Star
DOI: 10.3847/1538-4357/abe871 Bibcode: 2021ApJ...911...51L

Duev, Dmitry A.; Riddle, Reed; Mróz, Przemek +19 more

HO Puppis (HO Pup) was considered as a Be-star candidate based on its γ Cassiopeiae-type light curve, but lacked spectroscopic confirmation. Using distance measured from Gaia Data Release 2 and the spectral-energy-distribution fit on broadband photometry, the Be-star nature of HO Pup is ruled out. Furthermore, based on the 28,700 photometric data …

2021 The Astrophysical Journal
Gaia 11
The Nature of HI-absorption-selected Galaxies at z ≈ 4
DOI: 10.3847/1538-4357/ac12d2 Bibcode: 2021ApJ...921...68K

Prochaska, J. X.; Revalski, M.; Rafelski, M. +3 more

We report a Karl G. Jansky Very Large Array (JVLA) search for redshifted CO(1-0) or CO(2-1) emission, and a Hubble Space Telescope Wide Field Camera 3 (HST-WFC3) search for rest-frame near-ultraviolet (NUV) stellar emission, from seven HI-selected galaxies associated with high-metallicity ([M/H] ≥ -1.3) damped Lyα absorbers (DLAs) at z ≈ 4. The ga…

2021 The Astrophysical Journal
Gaia eHST 11
The First Extensive Exploration of UV-bright Stars in the Globular Cluster NGC 2808
DOI: 10.3847/1538-4357/abd2b5 Bibcode: 2021ApJ...908...66P

Sahu, Snehalata; Subramaniam, Annapurni; Prabhu, Deepthi S.

In this study, we identified and characterized the hot and luminous UV-bright stars in the globular cluster NGC 2808. We combined data from the Ultra Violet Imaging Telescope (UVIT) on board the Indian space satellite AstroSat with the Hubble Space Telescope UV Globular Cluster Survey data for the central region (within $\sim 2\buildrel{\,\prime}\…

2021 The Astrophysical Journal
Gaia eHST 11
Optical Identification and Spectroscopy of Supernova Remnants in the Galaxy M51
DOI: 10.3847/1538-4357/abd77d Bibcode: 2021ApJ...908...80W

Blair, William P.; Long, Knox S.; Winkler, P. Frank +2 more

Using a combination of ground-based and Hubble Space Telescope imaging, we have constructed a catalog of 179 supernova remnants (SNRs) and SNR candidates in the nearby spiral galaxy M51. Follow-up spectroscopy of 66 of the candidates confirms that 61 of these are SNRs and suggests that the vast majority of the unobserved objects are SNRs as well. …

2021 The Astrophysical Journal
Gaia eHST 11