Search Publications

Kpc-scale properties of dust temperature in terms of dust mass and star formation activity
DOI: 10.1093/mnras/stad373 Bibcode: 2023MNRAS.520.5506C

Sandstrom, Karin M.; Leroy, Adam K.; Rosolowsky, Erik +7 more

We investigate how dust temperature is affected by local environmental quantities, especially dust surface density (Σdust), dust-to-gas ratio (D/G), and interstellar radiation field. We compile multiwavelength observations in 46 nearby galaxies, uniformly processed with a common physical resolution of 2 kpc. A physical dust model is use…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 5
SOFIA FEEDBACK Survey: The Pillars of Creation in [C II] and Molecular Lines
DOI: 10.3847/1538-3881/acff6c Bibcode: 2023AJ....166..240K

Wyrowski, Friedrich; Tiwari, Maitraiyee; Güsten, Rolf +11 more

We investigate the physical structure and conditions of photodissociation regions (PDRs) and molecular gas within the Pillars of Creation in the Eagle Nebula using SOFIA FEEDBACK observations of the [C II] 158 µm line. These observations are velocity resolved to 0.5 km s-1 and are analyzed alongside a collection of complimentary d…

2023 The Astronomical Journal
JWST 5
The Binary and the Disk: The Beauty is Found within NGC3132 with JWST
DOI: 10.3847/1538-4357/aca7ba Bibcode: 2023ApJ...943..110S

Sahai, Raghvendra; Bujarrabal, Valentin; Quintana-Lacaci, Guillermo +4 more

The planetary nebula (PN) NGC 3132 is a striking example of the dramatic but poorly understood mass-loss phenomena that (1-8) M stars undergo during their death throes as they evolve into white dwarfs (WDs). From an analysis of JWST multiwavelength (0.9-18 µm) imaging of NGC 3132, we report the discovery of an extended dust clou…

2023 The Astrophysical Journal
Gaia eHST JWST 5
Novae in M51: a new, much higher rate from multi-epoch HST data
DOI: 10.1093/mnras/stac2960 Bibcode: 2023MNRAS.518.5279M

van Dokkum, Pieter; Conroy, Charlie; Shara, Michael M. +2 more

Accurate determination of the rates of nova eruptions in different kinds of galaxies gives us strong constraints on those galaxies' underlying white dwarf and binary populations, and those stars' spatial distributions. Until 2016, limitations inherent in ground-based surveys of external galaxies - and dust extinction in the Milky Way - significant…

2023 Monthly Notices of the Royal Astronomical Society
eHST 5
The Direction of the Flow of Interstellar Neutral H Based on Photometric Observations from SOHO/SWAN
DOI: 10.3847/1538-4357/acda8c Bibcode: 2023ApJ...952....2B

Bzowski, M.; Quémerais, E.; Kubiak, M. A. +3 more

Interstellar neutral hydrogen flows into the heliosphere as a mixture of the primary and secondary populations from two somewhat different directions due to splitting occurring in the magnetized outer heliosheath. The direction of the inflow of interstellar neutral H observed in the inner heliosphere, confronted with that of the unperturbed flow o…

2023 The Astrophysical Journal
SOHO 5
HST/WFC3 Light Curve Supports a Terrestrial Composition for the Closest Exoplanet to Transit an M Dwarf
DOI: 10.3847/1538-3881/acf561 Bibcode: 2023AJ....166..171P

Winters, Jennifer G.; Eastman, Jason D.; Bean, Jacob L. +6 more

Previous studies of the exoplanet LTT 1445Ac concluded that the light curve from the Transiting Exoplanet Survey Satellite (TESS) was consistent with both grazing and nongrazing geometries. As a result, the radius and hence density of the planet remained unknown. To resolve this ambiguity, we observed the LTT 1445 system for six spacecraft orbits …

2023 The Astronomical Journal
Gaia eHST 5
Searching for ejected supernova companions in the era of precise proper motion and radial velocity measurements
DOI: 10.1093/mnras/stad1054 Bibcode: 2023MNRAS.522.2029C

Lyman, J. D.; Groot, P. J.; Wiersema, K. +7 more

The majority of massive stars are born in binaries, and most unbind upon the first supernova. With precise proper motion surveys such as Gaia, it is possible to trace back the motion of stars in the vicinity of young remnants to search for ejected companions. Establishing the fraction of remnants with an ejected companion, and the photometric and …

2023 Monthly Notices of the Royal Astronomical Society
Gaia 5
A review of planetary systems around HD 99492, HD 147379, and HD 190007 with HARPS-N
DOI: 10.1051/0004-6361/202346887 Bibcode: 2023A&A...678A..90S

Poretti, E.; Sozzetti, A.; Delisle, J. -B. +26 more

Context. The Rocky Planet Search (RPS) program is dedicated to a blind radial velocity (RV) search of planets around bright stars in the northern hemisphere, using the high-resolution echelle spectrograph HARPS-N installed on the Telescopio Nazionale Galileo (TNG).
Aims: The goal of this work is to revise and update the properties of three pl…

2023 Astronomy and Astrophysics
Gaia 5
ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-Ray-detected Active Galactic Nuclei
DOI: 10.3847/1538-4357/acb4e9 Bibcode: 2023ApJ...945..121U

Fujimoto, Seiji; Kohno, Kotaro; Sun, Fengwu +10 more

We report the multiwavelength properties of millimeter galaxies hosting X-ray detected active galactic nuclei (AGNs) from the ALMA Lensing Cluster Survey (ALCS). ALCS is an extensive survey of well-studied lensing clusters with ALMA, covering an area of 133 arcmin2 over 33 clusters with a 1.2 mm flux-density limit of ~60 µJy (1σ).…

2023 The Astrophysical Journal
Herschel eHST 5
High-resolution spectroscopic analysis of four new chemically peculiar stars
DOI: 10.1093/mnras/stac3378 Bibcode: 2023MNRAS.518.5414R

Pereira, C. B.; Sneden, C.; Drake, N. A. +3 more

We present detailed chemical compositions of four stars on the first-ascent red giant branch that are classified as chemically peculiar, but lack comprehensive analyses at high spectral resolution. For BD+03°2688, HE 0457-1805, HE 1255-2324, and HE 2207-1746, we derived metallicities [Fe/H] = -1.21, -0.19, -0.31, and -0.55, respectively, indicatin…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 5