Article
Astronomy & Astrophysics
Vincenzo Ripepi, Laurent Chemin, Roberto Molinaro, Maria-Rosa L. Cioni, Kenji Bekki, Gisella Clementini, Richard de Grijs, Giulia De Somma, Dalal El Youssoufi, Leo Girardi, Martin A. T. Groenewegen, Valentin Ivanov, Marcella Marconi, Paul J. McMillan, Jacco Th van Loon
Summary: We analyzed the Y, J, and K-s light curves of delta Cepheid stars (DCEPs) in the Large Magellanic Cloud (LMC) using the VISTA near-infrared YJK(s) survey. We found a break in the period-luminosity and period-Wesenheit PW relationships for 1O DCEPs at P = 0.58 d. By calculating the individual distances of DCEPs in the LMC, we determined the position angle and inclination of the galaxy. Additionally, we observed non-planar distribution and a flared, thick disc structure in the LMC.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
V Ripepi, G. Catanzaro, R. Molinaro, M. Gatto, G. De Somma, M. Marconi, M. Romaniello, S. Leccia, I Musella, E. Trentin, G. Clementini, V Testa, F. Cusano, J. Storm
Summary: Classical Cepheids are crucial for the extragalactic distance scale, with their period-luminosity and period-Wesenheit relations showing dependency on metallicity. This metallicity dependence significantly affects the intercept of the PLZ/PWZ relations, indicating a larger impact than previously thought. However, it remains inconclusive whether the slope of these relationships also depends on metallicity. The correction of Gaia parallaxes' zero-point offset reduces the size of metallicity dependence on the PLZ/PWZ relations.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
V. V. Bobylev, A. T. Bajkova, A. S. Rastorguev, M. Zabolotskikh
Summary: This passage discusses constructing the rotation curve of the Galaxy using data on classical Cepheids, as well as analyzing the velocities of young and old Cepheids to determine the parameters of the spiral density wave. Spectral analysis reveals the ranges of parameters for the spiral density wave, with significant differences observed between young and old Cepheids. Integrating the orbits of old Cepheids backward in time allows for more reliable values of the spiral density wave parameters to be determined.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
V. Ripepi, G. Catanzaro, L. Molnar, E. Plachy, M. Marconi, G. Clementini, R. Molinaro, G. De Somma, S. Leccia, S. Mancino, I. Musella, F. Cusano, V. Testa
Summary: Classical Cepheids like Polaris and HD344787 are likely at their first crossing of the instability strip, with similar metal abundance Z=0.008. Differences in their properties during the main-sequence phase may explain variations seen in the Hertzsprung-Russell diagram.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Ilaria Musella, Marcella Marconi, Roberto Molinaro, Giuliana Fiorentino, Vincenzo Ripepi, Giulia De Somma, Maria Ida Moretti
Summary: ULPs are hypothesized as extensions of Classical Cepheids with longer periods, higher masses, and luminosities. They have potential as standard candles for cosmological measurements, but more data and theoretical support are needed for conclusive results.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
R. Molinaro, V. Ripepi, M. Marconi, M. Romaniello, G. Catanzaro, F. Cusano, G. De Somma, I. Musella, J. Storm, E. Trentin
Summary: Classical Cepheids are important for measuring distances in galaxies. The Gaia mission provides accurate parallaxes to calibrate these measurements. This study uses an implicit method to determine the zero point correction for Gaia parallaxes, finding a value of -22 +/- 4 mu as, in agreement with previous literature.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
G. Csoernyei, L. Szabados, L. Molnar, B. Cseh, N. Egei, Cs Kalup, V Kecskemethy, R. Koenyves-Toth, K. Sarneczky, R. Szakats
Summary: Investigating the period changes of classical Cepheids through the framework of O - C diagrams provides insights into their evolution and nature. This study presents new or extended O - C diagrams for 148 Galactic classical Cepheids, and finds observational indications of period change rate dependence on the horizontal position within the instability strip. Period fluctuations are observed in 59 Cepheids, which are uniformly distributed over the inspected period range. The fluctuation amplitude is found to be dependent on the pulsation period, similar to longer period pulsating variable stars.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
E. Trentin, V Ripepi, G. Catanzaro, J. Storm, M. Marconi, G. De Somma, V Testa, I Musella
Summary: This article examines the faintest classical Cepheids in the Milky Way, deriving atmospheric parameters, radial velocities, and abundances for each star. By comparing the data with previous studies, the authors find a metallicity gradient in the Galactic disc and a possible break in the gradient at R-GC = 9.25 kpc.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
V Lebouteiller, L. Ramambason
Summary: This study presents a probabilistic approach to infer the properties of the interstellar medium in high-redshift galaxies. The authors use a Bayesian method and statistical framework, combining multiple probabilistic concepts and models, to infer the probability distributions of several physical parameters in the metal-poor dwarf galaxy I Zw 18. The results show that this method can provide accurate results and contribute to the understanding of galaxy evolution and star formation processes.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Jason L. Sanders
Summary: Gaia DR3 parallaxes are used to calibrate preliminary period-luminosity relations of O-rich Mira variables. The derived relations are compared to those measured for different celestial objects. Models of the Gaia astrometry for the Mira variables suggest that the recovered parallaxes should be unbiased but with underestimated uncertainties for the nearest stars. The derived period-luminosity relations are used to find the Hubble constant for the Type Ia host galaxy NGC 1559.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
E. S. G. de Almeida, M. Hugbart, A. Domiciano de Souza, J-P Rivet, F. Vakili, A. Siciak, G. Labeyrie, O. Garde, N. Matthews, O. Lai, D. Vernet, R. Kaiser, W. Guerin
Summary: This paper reports on spatial intensity interferometry measurements of two stars, P Cygni and Rigel, using an upgraded experimental setup and radiative transfer models. The study successfully determined the distances of these stars and found agreement with previous measurements. This research is significant for extending the application of the Wind Momentum Luminosity Relation method for distance calibration.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Richard Anderson
Summary: This study estimates relativistic corrections for cosmic distance estimates based on stellar standard candles to achieve an unbiased 1% measurement of Hubble's constant in the future. The results suggest that all stellar standard candle observations require relativistic corrections for accurate distance measurements.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
M. E. Ridder, C. O. Heinke, G. R. Sivakoff, A. K. Hughes
Summary: We report two new radio detections of cataclysmic variables (CVs) and compare them with other CVs detected by radio and X-ray. The radio luminosities of these systems are unexpectedly high and their origin remains a puzzle. The radio emission mechanism for these CVs may be electron-cyclotron maser emission, synchrotron radiation, or a more exotic process. The locations of these CVs in the radio-X-ray luminosity plane suggest additional complexity in classifying unknown systems based on their radio and X-ray luminosities alone.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Zhaozhou An, Sergey E. Koposov
Summary: We studied the 3D structure of five dwarf galaxies using BHB stars as distance indicators. By constructing a new color-absolute magnitude of BHB stars and through modeling, we found statistically significant non-zero gradients in Sextans and Sculptor dwarf galaxies, and the distance gradients in these two galaxies are inconsistent with prolate shape.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
G. Csoernyei, R. I. Anderson, C. Vogl, S. Taubenberger, S. Blondin, B. Leibundgut, W. Hillebrandt
Summary: This study estimates the distance to the Whirlpool galaxy, M 51, using two independent methods: Cepheid variables and the expanding photosphere method. The resulting distance estimates are 7.59 Mpc and 7.34 Mpc respectively, which are more precise than previous estimates. This finding highlights the importance of direct cross-checks between independent distance estimates.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Mirko Curti, Francesco D'Eugenio, Stefano Carniani, Roberto Maiolino, Lester Sandles, Joris Witstok, William M. Baker, Jake S. Bennett, Joanna M. Piotrowska, Sandro Tacchella, Stephane Charlot, Kimihiko Nakajima, Gabriel Maheson, Filippo Mannucci, Amirnezam Amiri, Santiago Arribas, Francesco Belfiore, Nina R. Bonaventura, Andrew J. Bunker, Jacopo Chevallard, Giovanni Cresci, Emma Curtis-Lake, Connor Hayden-Pawson, Gareth C. Jones, Nimisha Kumari, Isaac Laseter, Tobias J. Looser, Alessandro Marconi, Michael Maseda, Jan Scholtz, Renske Smit, Hannah Ubler, Imaan E. B. Wallace
Summary: We analyze the chemical properties of three z similar to 8 galaxies behind the galaxy cluster SMACSJ0723.3-7327 and measure their metallicities using the direct T-e method for the first time at such high redshift. The galaxies show different excitation properties compared to local strong-line metallicity calibrations, suggesting a need for reassessment of the calibrations at these redshifts. The two galaxies at z similar to 7.6 have metallicities consistent with the extrapolation of the mass-metallicity relation, while the least massive galaxy at z similar to 8.5 shows a significantly lower metallicity, indicating a deviation from the equilibrium between gas flows, star formation, and metal enrichment.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
G. A. Matzeu, M. Brusa, G. Lanzuisi, M. Dadina, S. Bianchi, G. Kriss, M. Mehdipour, E. Nardini, G. Chartas, R. Middei, E. Piconcelli, V. Gianolli, A. Comastri, A. L. Longinotti, Y. Krongold, F. Ricci, P. O. Petrucci, F. Tombesi, A. Luminari, L. Zappacosta, G. Miniutti, M. Gaspari, E. Behar, M. Bischetti, S. Mathur, M. Perna, M. Giustini, P. Grandi, E. Torresi, C. Vignali, G. Bruni, M. Cappi, E. Costantini, G. Cresci, B. De Marco, A. De Rosa, R. Gilli, M. Guainazzi, J. Kaastra, S. Kraemer, F. La Franca, A. Marconi, F. Panessa, G. Ponti, D. Proga, F. Ursini, P. Baldini, F. Fiore, A. R. King, R. Maiolino, G. Matt, A. Merloni
Summary: We present a new X-ray spectroscopic study of 22 luminous AGNs at intermediate redshifts, focusing on the search for and characterization of ultra-fast outflows (UFOs). Through Monte Carlo procedures, we confirm the detection of highly ionized iron absorption lines in 7 out of 22 sources at a high confidence level, supporting the existence of highly ionized matter propagating at mildly relativistic speeds in a considerable fraction of AGNs. The SUpermassive Black hole Winds in the x-rAYS (SUBWAYS) campaign extends previous studies on Seyferts and finds a UFO detection fraction of approximately 30% of the total sample.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
I. Saccheo, A. Bongiorno, E. Piconcelli, V. Testa, M. Bischetti, S. Bisogni, G. Bruni, G. Cresci, C. Feruglio, F. Fiore, A. Grazian, A. Luminari, E. Lusso, V. Mainieri, R. Maiolino, A. Marconi, F. Ricci, F. Tombesi, A. Travascio, G. Vietri, C. Vignali, L. Zappacosta, F. La Franca
Summary: The aim of this study is to investigate the mean spectral energy distribution (SED) of a sample of 85 WISE-SDSS selected hyperluminous quasars (WISSH) and compare them to less luminous sources. The results show that hyperluminous quasars have a lower X-ray emission and an excess in the near- and mid-IR, possibly due to a larger dust contribution. The study also finds that quasars with broad absorption lines have weaker X-ray emission and stronger emission from the hot dust component.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
A. Marasco, F. Belfiore, G. Cresci, F. Lelli, G. Venturi, L. K. Hunt, A. Concas, A. Marconi, F. Mannucci, M. Mingozzi, A. F. McLeod, N. Kumari, S. Carniani, L. Vanzi, M. Ginolfi
Summary: By observing and modeling a sample of 19 galaxies with stellar masses ranging from 10⁷ to 10¹⁰ solar masses, it is found that the ionized gas in these galaxies exhibits non-circular motion and low mass outflow rates, which significantly deviate from the predictions of theoretical models. This suggests that baryonic feedback plays a gentle gas cycling role rather than causing large-scale blow-outs in low-mass galaxies.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
D. O. Cook, J. C. Lee, A. Adamo, D. Calzetti, R. Chandar, B. C. Whitmore, A. Aloisi, M. Cignoni, D. A. Dale, B. G. Elmegreen, M. Fumagalli, K. Grasha, K. E. Johnson, R. C. Kennicutt, H. Kim, S. T. Linden, M. Messa, G. Ostlin, J. E. Ryon, E. Sacchi, D. A. Thilker, M. Tosi, A. Wofford
Summary: We studied the relationship between the properties of young star clusters and their host galaxies in 23 dwarf and irregular galaxies observed by the Hubble Space Telescope (HST) Legacy ExtraGalactic Ultraviolet Survey (LEGUS). We found that there were no significant correlations between the properties of the star clusters and the star formation rate (SFR) density of the host galaxies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
A. Ciurlo, F. Mannucci, S. Yeh, A. Amiri, S. Carniani, C. Cicone, G. Cresci, E. Lusso, A. Marasco, C. Marconcini, A. Marconi, E. Nardini, E. Pancino, P. Rosati, K. Rubinur, P. Severgnini, M. Scialpi, G. Tozzi, G. Venturi, C. Vignali, M. Volonteri
Summary: The existence of multiple AGNs at small projected distances on the sky is important for addressing astrophysical and cosmological questions. The newly developed Gaia multi-peak method has provided numerous new candidate members of these populations. Spatially resolved spectroscopy confirms the presence of multiple AGNs in four GMP-selected candidates, doubling the number of confirmed multiple AGNs at projected separations below 7 kpc at z > 0.5 and presenting the first detection of a possible triple AGN.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
E. Parlanti, S. Carniani, A. Pallottini, M. Cignoni, G. Cresci, M. Kohandel, F. Mannucci, A. Marconi
Summary: A study finds that in the first billion years of the Universe, the gas kinematics of high-redshift galaxies are similar to local galaxies, with rotating but turbulent disks.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
G. Cresci, G. Tozzi, M. Perna, M. Brusa, C. Marconcini, A. Marconi, S. Carniani, M. Brienza, M. Giroletti, F. Belfiore, M. Ginolfi, F. Mannucci, L. Ulivi, J. Scholtz, G. Venturi, S. Arribas, H. Ubler, F. D'Eugenio, M. Mingozzi, B. Balmaverde, A. Capetti, E. Parlanti, T. Zana
Summary: This study presents the first direct observational evidence of powerful outflows around a heavily obscured supermassive black hole at a redshift of 1.59, confirming the role of quasar feedback in suppressing star formation in galaxies. The results reveal the complex interplay between AGN jets, winds, and the interstellar medium of the host galaxy, highlighting the significance of NIRSpec in studying feedback mechanisms at high redshift.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Mattia Libralato, Andrea Bellini, Roeland P. van der Marel, Jay Anderson, Sangmo Tony Sohn, Laura L. Watkins, Lili Alderson, Natalie Allen, Mark Clampin, Ana Glidden, Jayesh Goyal, Kielan Hoch, Jingcheng Huang, Jens Kammerer, Nikole K. Lewis, Zifan Lin, Douglas Long, Dana Louie, Ryan J. MacDonald, Matt Mountain, Maria Pena-Guerrero, Marshall D. Perrin, Laurent Pueyo, Isabel Rebollido, Emily Rickman, Sara Seager, Kevin B. Stevenson, Jeff A. Valenti, Daniel Valentine, Hannah R. Wakeford
Summary: We develop and disseminate effective point-spread functions and geometric-distortion solutions for high-precision astrometry and photometry with the JWST NIRISS instrument. We correct field dependencies and detector effects, and assess the quality and the temporal stability of the calibrations. As a scientific application and validation, we study the proper motion (PM) kinematics of stars in the JWST calibration field near the Large Magellanic Cloud (LMC) center, comparing to a first-epoch Hubble Space Telescope (HST) archival catalog with a 16 yr baseline.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Mattia Libralato, Enrico Vesperini, Andrea Bellini, Antonino P. Milone, Roeland P. van der Marel, Giampaolo Piotto, Jay Anderson, Antonio Aparicio, Beatriz Barbuy, Luigi R. Bedin, Thomas M. Brown, Santi Cassisi, Domenico Nardiello, Ata Sarajedini, Michele Scalco
Summary: Our understanding of the kinematic properties of multiple stellar populations (mPOPs) in Galactic globular clusters (GCs) is limited. We analyzed 56 GCs using high-precision proper motions computed with Hubble Space Telescope data. We found that 1G stars are generally kinematically isotropic, while 2G stars are isotropic at the center and become radially anisotropic before the half-light radius. The radial anisotropy is induced by a lower tangential velocity dispersion of 2G stars with respect to the 1G population.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Anupam Bhardwaj, Marcella Marconi, Marina Rejkuba, Richard de Grijs, Harinder P. P. Singh, Vittorio F. F. Braga, Shashi Kanbur, Chow-Choong Ngeow, Vincenzo Ripepi, Giuseppe Bono, Giulia De Somma, Massimo Dall'Ora
Summary: We empirically measure the distances of RR Lyrae stars using near-infrared monitoring of Galactic globular clusters and find a significant dependence of their near-infrared period-luminosity relationships on metallicity. The metallicity coefficients and zero-points of the empirical relationships are consistent with theoretical predictions, and the RR Lyrae-based distances to the globular clusters are consistent with other independent measurements.
ASTROPHYSICAL JOURNAL LETTERS
(2023)
Article
Astronomy & Astrophysics
M. Di Criscienzo, S. Leccia, V. Braga, I. Musella, G. Bono, M. Dall'Ora, G. Fiorentino, M. Marconi, R. Molinaro, V. Ripepi, K. Carrell, Y. Choi, S. Savarese, L. Schreiber
Summary: This investigation focuses on the LSST Survey Strategy Optimization process and the development of a new tool called PulsationStarRecovery. It demonstrates the importance of excellent recovery in understanding the potential of LSST in using pulsating stars as stellar tracers and distance indicators. The study also shows the difference in recovery based on distance and variable-star type.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2023)
Article
Astronomy & Astrophysics
Giulia Tozzi, Roberto Maiolino, Giovanni Cresci, Joanna M. Piotrowska, Francesco Belfiore, Mirko Curti, Filippo Mannucci, Alessandro Marconi
Summary: The He ii lambda 4686 angstrom line emission can be used to identify active galactic nuclei (AGN) in actively star-forming (SF) galaxies, which are typically missed by the standard BPT classification. In this study, we used spatially resolved data from the MaNGA DR15 survey to identify hidden AGN in the Local Universe. By combining results from He ii and BPT diagnostics, we found that 10% of the galaxies in MaNGA DR15 are AGN host candidates, out of which 27 are identified as AGN using the He ii diagram only. This population of He ii-only AGN is hosted by massive SF Main Sequence galaxies and is less luminous on average compared to the BPT-selected AGN.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
D. Kakkad, V Mainieri, G. Vietri, I Lamperti, S. Carniani, G. Cresci, C. Harrison, A. Marconi, M. Bischetti, C. Cicone, C. Circosta, B. Husemann, A. Man, F. Mannucci, H. Netzer, P. Padovani, M. Perna, A. Puglisi, J. Scholtz, G. Tozzi, C. Vignali, L. Zappacosta
Summary: We present the spatially resolved H alpha properties of 21 type 1 AGN host galaxies at z similar to 2 derived from the SUPER survey. We find extended H alpha emission in 16 out of the 21 type 1 AGN host galaxies (76 per cent). Based on the BPT diagnostics, optical line flux ratios, and line widths, we show that the H alpha emission in five galaxies is ionized by the AGN (30 per cent), in four galaxies by star formation (25 per cent), and for the rest (45 per cent), the ionization source is unconstrained. Two galaxies show extended H alpha FWHM >600 km s(-1), which is interpreted as a part of an AGN-driven outflow.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
W. Cerny, A. Drlica-Wagner, T. S. Li, A. B. Pace, K. A. G. Olsen, N. E. D. Noel, R. P. van der Marel, J. L. Carlin, Y. Choi, D. Erkal, M. Geha, D. J. James, C. E. Martinez-Vazquez, P. Massana, G. E. Medina, A. E. Miller, B. Mutlu-Pakdil, D. L. Nidever, J. D. Sakowska, G. S. Stringfellow, J. A. Carballo-Bello, P. S. Ferguson, N. Kuropatkin, S. Mau, E. J. Tollerud, A. K. Vivas, DELVE Collaboration
Summary: We discovered DELVE 6, an ultra-faint stellar system in the second data release of the DECam Local Volume Exploration (DELVE) survey. DELVE 6 is an old and metal-poor stellar system with certain physical properties consistent with other ultra-faint star clusters. It is located near the Small Magellanic Cloud (SMC) and potentially associated with the SMC/LMC.
ASTROPHYSICAL JOURNAL LETTERS
(2023)