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When determining absolute ages of identifiably young stellar populations, results strongly depend on which stars are studied. Cooler (K, M) stars typically yield ages that are systematically younger than warmer (A, F, G) stars by a factor…

Solar and Stellar Astrophysics · Physics 2016-10-05 Gregory A. Feiden

The detection of $\sim 1.5-3.2$ Myr old $^{60}$Fe on Earth indicates recent nearby core-collapse supernovae. For supernovae in multiple stars, the primary stars may become neutron stars, while former companions may become unbound and become…

High Energy Astrophysical Phenomena · Physics 2019-10-02 Ralph Neuhaeuser , Frank Gießler , Valeri V. Hambaryan

A set of 41 nearby stars (closer than 25 pc) is investigated which have very wide binary and common proper motion (CPM) companions at projected separations between 1000 and $200 000$ AU. These companions are identified by astrometric…

Astrophysics · Physics 2009-11-13 V. V. Makarov , N. Zacharias , G. S. Hennessy

Using the near-infrared spectrometer SpeX and its slit-viewing camera at the IRTF, I have resolved a low-mass member of the Upper Scorpius OB association into a double star. From K-band images of the pair, DENIS-P J161833.2-251750.4 A and…

Astrophysics · Physics 2009-11-13 K. L. Luhman

We analyze the optical counterpart to the ultra-compact high velocity cloud AGC 226067, utilizing imaging taken with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope. The color magnitude diagram of the main body of AGC…

The HR 1614 overdensity in velocity space and has for a long time been known as an old (~2 Gyr) and metal-rich ([Fe/H]~0.2) nearby moving group that has a dissolving cluster origin. The existence of such old and metal-rich groups in the…

Astrophysics of Galaxies · Physics 2020-07-01 Iryna Kushniruk , Thomas Bensby , Sofia Feltzing , Christian L. Sahlholdt , Diane Feuillet , Luca Casagrande

We study X-ray emission from young stars by analyzing deep XMM-Newton observations of two regions of the Upper Scorpius association, having an age of 5 Myr. Based on near infrared and optical photometry we identify 22 Upper Scorpius…

Astrophysics · Physics 2009-11-11 C. Argiroffi , F. Favata , E. Flaccomio , A. Maggio , G. Micela , G. Peres , S. Sciortino

We present deep 1.2 millimeter photometry of 37 stars in the young (5 Myr) Upper Scorpius OB association, sensitive to ~4 x 10^-3 Mjup of cool millimeter dust. Disks around four low- and solar-mass stars are detected, as well as one debris…

Solar and Stellar Astrophysics · Physics 2015-06-03 Geoffrey S. Mathews , Jonathan P. Williams , Francois Ménard , Neil Phillips , Gaspard Duchêne , Christophe Pinte

We present results of an infrared study of the molecular cloud Lynds 1340, forming three groups of low and intermediate-mass stars. Our goals are to identify and characterise the young stellar population of the cloud, study the…

Solar and Stellar Astrophysics · Physics 2016-06-09 M. Kun , G. Wolf-Chase , A. Moór , D. Apai , Z. Balog , J. O'Linger-Luscusk , G. Moriarty-Schieven

Architecture and parameters of two wide nearby hierarchical systems containing five solar-type stars each, $\kappa$ Tuc and $\xi$ Sco, are studied. Using Gaia astrometry and photometry, masses are determined from visual orbits and…

Solar and Stellar Astrophysics · Physics 2021-01-11 Andrei Tokovinin

The paper presents results from a small survey of 22 young, nearby stars that was designed to detect substellar companions and ultimately giant extrasolar planets down to Jupiter masses. The targets are members of the Tucana and Beta…

Astrophysics · Physics 2009-11-13 Markus Kasper , Daniel Apai , Markus Janson , Wolfgang Brandner

We have observed 22 Lindroos stars with SCUBA on the JCMT to search for evidence of dust discs. Stars in this sample are the less massive companions of B-type primaries and have ages of 10-170Myr. Dust was detected around three of these…

Astrophysics · Physics 2009-11-07 M. C. Wyatt , W. R. F. Dent , J. S. Greaves

We aim at constraining evolutionary models at low mass and young ages by identifying interesting transiting system members of the nearest OB association to the Sun, Upper Scorpius, targeted by the Kepler mission. We produced light curves…

We present revised stellar ages for 23 pre-main sequence K- and M-type stars in the Upper Scorpius star-forming region, derived by using stellar dynamical masses to constrain isochronal ages from five pre-main sequence stellar evolutionary…

Astrophysics of Galaxies · Physics 2026-02-02 Allison P. M. Towner , Joshua A. Eisner , Patrick D. Sheehan , Lynne D. Hillenbrand , Ya-Lin Wu

Presented here are 442 new proper motion stellar systems in the southern sky between declinations -$90\degr$ and -47$\degr$ with 0$\farcs$40 yr$^{-1}$ $>$ $\mu$ $\ge$ 0$\farcs$18 yr$^{-1}$. These systems constitute a 25.3% increase in new…

Solar and Stellar Astrophysics · Physics 2015-05-19 Charlie T. Finch , Norbert Zacharias , Todd J. Henry

We present an investigation of the relationship between giant molecular cloud (GMC) properties and the associated stellar clusters in the nearby flocculent galaxy NGC 7793. We combine the star cluster catalog from the HST LEGUS (Legacy…

We present NIR and MIR observations of eight embedded young stellar groups around Herbig Ae/Be stars (HAEBEs) using archived Spitzer IRAC data and 2MASS data. These young stellar groups are nearby ($\leq$ 1 kpc) and still embedded within…

Astrophysics · Physics 2011-02-11 Shiya Wang , Leslie W. Looney

We report the results of a spatially compete, high-sensitivity survey for Herbig-Haro (HH) outflows in the Western and Eastern Circinus molecular clouds. We have detected 28 new HH objects in Circinus West, doubling the number known in this…

Astrophysics of Galaxies · Physics 2025-03-20 T. A. Rector , L. Prato , R. Kerr , E. Papraniku , K. Fisk

(Abridged) Our aim is to identify analogues of gas giant planets, as companions at wide separations of very young stars. To identify these objects, we cross correlated the Visible and Infrared Survey Telescope for Astronomy (VISTA)…