Search Publications

The Radiation Environments of Middle-aged F-type Stars
DOI: 10.3847/1538-4357/aced9f Bibcode: 2023ApJ...956...79C

France, K.; Hinton, P. C.; Fleming, B. +5 more

Far-ultraviolet (FUV) emission lines from dwarf stars are important driving sources of photochemistry in planetary atmospheres. Properly interpreting spectral features of planetary atmospheres critically depends on the emission of its host star. While the spectral energy distributions (SEDs) of K- and M-type stars have been extensively characteriz…

2023 The Astrophysical Journal
Gaia IUE eHST 2
Accretion Disk Wind of Hercules X-1 during the Short High State
DOI: 10.3847/1538-4357/acfc3e Bibcode: 2023ApJ...959...51K

Fabian, A. C.; Pinto, C.; Kara, E. +5 more

Hercules X-1 is a nearly edge-on X-ray binary with a warped, precessing accretion disk, which manifests through a 35-day cycle of alternating High and Low flux states. This disk precession introduces a changing line of sight toward the X-ray source, through an ionized accretion disk wind. The sightline variation allows us to uniquely determine how…

2023 The Astrophysical Journal
XMM-Newton 2
A Broad-line Quasar with Unexplained Extreme Velocity Offsets: Post-shock Outflow?
DOI: 10.3847/1538-4357/acadd8 Bibcode: 2023ApJ...944..217R

Schramm, Malte; Mobasher, Bahram; Steinhardt, Charles L. +4 more

The quasar SDSS 0956 + 5128 exhibits three distinct velocity components with large offsets in emission: the systemic velocity of [O II], [O III], and [Ne III] narrow lines have redshift z = 0.7142; the broad Mg II line is shifted by -1200 km s-1 with respect to the narrow lines; the broad Hα and Hβ lines are at -4100 km s-1. …

2023 The Astrophysical Journal
eHST 2
Strong Variability in AzV 493, an Extreme Oe-type Star in the SMC
DOI: 10.3847/1538-4357/acb690 Bibcode: 2023ApJ...947...27O

Oey, M. S.; Renzo, M.; Castro, N. +11 more

We present 18 yr of OGLE photometry together with spectra obtained over 12 yr revealing that the early Oe star AzV 493 shows strong photometric (ΔI < 1.2 mag) and spectroscopic variability with a dominant, 14.6 yr pattern and ~40 day oscillations. We estimate the stellar parameters T eff = 42,000 K, $\mathrm{log}L/{L}_{\odot }=5.83\p…

2023 The Astrophysical Journal
Gaia 2
A Search for X-Ray/UV Correlation in the Reflection-dominated Seyfert 1 Galaxy Markarian 1044
DOI: 10.3847/1538-4357/acf464 Bibcode: 2023ApJ...958...46B

Jithesh, V.; Medhi, Biman J.; Misra, Ranjeev +3 more

Correlated variability between coronal X-rays and disk optical/UV photons provides a very useful diagnostic of the interplay between the different regions around an active galactic nucleus (AGN) and how they interact. AGNs that reveal strong X-ray reflection in their spectra should normally exhibit optical/UV to X-ray correlation consistent with r…

2023 The Astrophysical Journal
XMM-Newton 2
Atmospheric Pressure and Molecular Cloud Formation in Early-type Galaxies
DOI: 10.3847/1538-4357/acb53f Bibcode: 2023ApJ...944...69B

McNamara, B. R.; Russell, H. R.; Edge, A. C. +3 more

A strong correlation between atmospheric pressure and molecular gas mass is found in central cluster galaxies and early-type galaxies. This trend and a similar trend with atmospheric gas density would naturally arise if the molecular clouds condensed from hot atmospheres. Limits on the ratio of molecular to atomic hydrogen in these systems exceed …

2023 The Astrophysical Journal
XMM-Newton 2
Transverse Vertical Oscillations During the Contraction and Expansion of Coronal Loops
DOI: 10.3847/1538-4357/acd5cf Bibcode: 2023ApJ...951..126Z

Li, Qiao; Zhang, Qingmin; Li, Chuan +5 more

In this paper, we carry out a detailed analysis of the M1.6 class eruptive flare occurring in NOAA active region 13078 on 2022 August 19. The flare is associated with a fast coronal mass ejection (CME) propagating in the southwest direction with an apparent speed of ~926 km s-1. Meanwhile, a shock wave is driven by the CME at the flank.…

2023 The Astrophysical Journal
SOHO 2
Angular Momentum Variation of the Milky Way Thick Disk: The Dependence of Chemical Abundance and Evidence of the Inside-out Formation Scenario
DOI: 10.3847/1538-4357/acd058 Bibcode: 2023ApJ...950..142H

Li, Lu; Hu, Guozhen; Shao, Zhengyi

We investigate the angular momentum of mono-abundance populations (MAPs) of the Milky Way thick disk by using a sample of 26,076 giant stars taken from APOGEE Data Release (DR) 17 and Gaia early DR3. The vertical and perpendicular angular momentum components, L Z and L P , of the MAPs in narrow bins have significant variat…

2023 The Astrophysical Journal
Gaia 2
Searching for the Role of Mergers in Fast and Early SMBH Growth: Morphological Decomposition of Quasars and Their Hosts at z 4.8
DOI: 10.3847/1538-4357/acebc9 Bibcode: 2023ApJ...955...15T

Trakhtenbrot, Benny; Simmons, Brooke D.; Netzer, Hagai +4 more

We present rest-frame ultraviolet images of six luminous quasars at z ~ 4.8 obtained with the Hubble Space Telescope (HST). These quasars exhibit a wide range of star formation rates (SFRs) and lie in a wide range of environments. We carefully model and subtract the point-like quasar emission and investigate the morphology of the underlying host g…

2023 The Astrophysical Journal
eHST 2
Gaia17bpp: A Giant Star with the Deepest and Longest Known Dimming Event
DOI: 10.3847/1538-4357/aceda7 Bibcode: 2023ApJ...955...69T

Davenport, James R. A.; Bellm, Eric C.; Tzanidakis, Anastasios +1 more

We report the serendipitous discovery of Gaia17bpp/2MASS J19372316+1759029, a binary star with a deep single large-amplitude dimming event of ~4.5 mag that lasted over 6.5 yr. Using the optical-to-IR spectral energy distribution (SED), we constrain the primary star to be a cool giant M0III star with effective temperature T eff = 3850 K …

2023 The Astrophysical Journal
Gaia 2