PSR J1306–40: An X-ray Luminous Redback with an Evolved Companion. (arXiv:1903.09211v1 [astro-ph.HE])

PSR J1306–40: An X-ray Luminous Redback with an Evolved Companion. (arXiv:1903.09211v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Swihart_S/0/1/0/all/0/1">Samuel J. Swihart</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Strader_J/0/1/0/all/0/1">Jay Strader</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chomiuk_L/0/1/0/all/0/1">Laura Chomiuk</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Shishkovsky_L/0/1/0/all/0/1">Laura Shishkovsky</a> PSR J1306–40 is a millisecond pulsar binary with a non-degenerate companion in an unusually long $sim$1.097 day orbit. We present new optical photometry and spectroscopy of this system, and model […]

The Weird Detector: Flagging periodic, coherent signals of arbitrary shape in time series photometry. (arXiv:1903.09213v1 [astro-ph.EP])

The Weird Detector: Flagging periodic, coherent signals of arbitrary shape in time series photometry. (arXiv:1903.09213v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Wheeler_A/0/1/0/all/0/1">Adam Wheeler</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kipping_D/0/1/0/all/0/1">David Kipping</a> By design, model-based approaches for flagging transiting exoplanets in light curves, such as boxed least squares, excel at detecting planets with low S/N at the expense of finding signals that are not well […]

Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes. (arXiv:1903.09220v1 [astro-ph.HE])

Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes. (arXiv:1903.09220v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Kalogera_V/0/1/0/all/0/1">Vassiliki Kalogera</a> (Northwestern U), <a href="http://arxiv.org/find/astro-ph/1/au:+Berry_C/0/1/0/all/0/1">Christopher P L Berry</a> (Northwestern U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Colpi_M/0/1/0/all/0/1">Monica Colpi</a> (U. of Milano-Bicocca), <a href="http://arxiv.org/find/astro-ph/1/au:+Fairhurst_S/0/1/0/all/0/1">Steve Fairhurst</a> (Cardiff U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Justham_S/0/1/0/all/0/1">Stephen Justham</a> (UCAS, Beijing and U. of Amsterdam), <a href="http://arxiv.org/find/astro-ph/1/au:+Mandel_I/0/1/0/all/0/1">Ilya Mandel</a> (Monash U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Mangiagli_A/0/1/0/all/0/1">Alberto Mangiagli</a> (U. of […]

Extreme Gravity and Fundamental Physics. (arXiv:1903.09221v1 [astro-ph.HE])

Extreme Gravity and Fundamental Physics. (arXiv:1903.09221v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Sathyaprakash_B/0/1/0/all/0/1">B.S. Sathyaprakash</a> (Penn State and Cardiff University), <a href="http://arxiv.org/find/astro-ph/1/au:+Bailes_M/0/1/0/all/0/1">Matthew Bailes</a> (Swinburne U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Kasliwal_M/0/1/0/all/0/1">Mansi M. Kasliwal</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Nissanke_S/0/1/0/all/0/1">Samaya Nissanke</a> (U. of Amsterdam), <a href="http://arxiv.org/find/astro-ph/1/au:+Anand_S/0/1/0/all/0/1">Shreya Anand</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Andreoni_I/0/1/0/all/0/1">Igor Andreoni</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Colpi_M/0/1/0/all/0/1">Monica Colpi</a> (U. of Milano – Bicocca), <a href="http://arxiv.org/find/astro-ph/1/au:+Coughlin_M/0/1/0/all/0/1">Michael Coughlin</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Hall_E/0/1/0/all/0/1">Evan Hall</a> (MIT), […]

The Yet-Unobserved Multi-Messenger Gravitational-Wave Universe. (arXiv:1903.09224v1 [astro-ph.HE])

The Yet-Unobserved Multi-Messenger Gravitational-Wave Universe. (arXiv:1903.09224v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Kalogera_V/0/1/0/all/0/1">Vassiliki Kalogera</a> (Northwestern U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Bizouard_M/0/1/0/all/0/1">Marrie-Anne Bizouard</a> (CNRS, OCA), <a href="http://arxiv.org/find/astro-ph/1/au:+Burrows_A/0/1/0/all/0/1">Adam Burrows</a> (Princeton U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Janka_T/0/1/0/all/0/1">Thomas Janka</a> (MPA), <a href="http://arxiv.org/find/astro-ph/1/au:+Kotake_K/0/1/0/all/0/1">Kei Kotake</a> (Fukuoka U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Messer_B/0/1/0/all/0/1">Bronson Messer</a> (ORNL &amp; U. Tennessee), <a href="http://arxiv.org/find/astro-ph/1/au:+Mezzacappa_T/0/1/0/all/0/1">Tony Mezzacappa</a> (ORNL &amp; U. Tennessee), <a href="http://arxiv.org/find/astro-ph/1/au:+Mueller_B/0/1/0/all/0/1">Bernhard Mueller</a> (Monash U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Mueller_E/0/1/0/all/0/1">Ewald Mueller</a> (MPA), <a […]

Messier 82 – the Cigar Galaxy

Messier 82 – the Cigar Galaxy Located in the vicinity Ursa Major constellation, roughly 12 million light years from Earth, is the starburst galaxy known as the Messier 82 (aka. the Cigar Galaxy). The post Messier 82 – the Cigar Galaxy appeared first on Universe Today. Universe Today Go to Source

Flaring, Dust Formation, And Shocks In The Very Slow Nova ASASSN-17pf (LMCN 2017-11a). (arXiv:1903.09232v1 [astro-ph.HE])

Flaring, Dust Formation, And Shocks In The Very Slow Nova ASASSN-17pf (LMCN 2017-11a). (arXiv:1903.09232v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Aydi_E/0/1/0/all/0/1">E. Aydi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chomiuk_L/0/1/0/all/0/1">L. Chomiuk</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Strader_J/0/1/0/all/0/1">J. Strader</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Swihart_S/0/1/0/all/0/1">S. J. Swihart</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bahramian_A/0/1/0/all/0/1">A. Bahramian</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Harvey_E/0/1/0/all/0/1">E. J. Harvey</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Britt_C/0/1/0/all/0/1">C. T. Britt</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Buckley_D/0/1/0/all/0/1">D. A. H. Buckley</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_P/0/1/0/all/0/1">P. Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dage_K/0/1/0/all/0/1">K. Dage</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Darnley_M/0/1/0/all/0/1">M. J. Darnley</a>, <a […]

Constraining the size of the corona with fully relativistic calculations of spectra of extended corona. I – the Monte Carlo radiative transfer code. (arXiv:1903.09241v1 [astro-ph.HE])

Constraining the size of the corona with fully relativistic calculations of spectra of extended corona. I – the Monte Carlo radiative transfer code. (arXiv:1903.09241v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_W/0/1/0/all/0/1">Wenda Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dovciak_M/0/1/0/all/0/1">Michal Dov&#x10d;iak</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bursa_M/0/1/0/all/0/1">Michal Bursa</a> The size and geometry of the X-ray emitting corona in AGNs are still not well constrained. Dovv{c}iak & Done (2016) proposed […]

Qatar Exoplanet Survey: Qatar-8b, 9b and 10b — A Hot Saturn and Two Hot Jupiters. (arXiv:1903.09258v1 [astro-ph.EP])

Qatar Exoplanet Survey: Qatar-8b, 9b and 10b — A Hot Saturn and Two Hot Jupiters. (arXiv:1903.09258v1 [astro-ph.EP]) <a href="http://arxiv.org/find/astro-ph/1/au:+Alsubai_K/0/1/0/all/0/1">Khalid Alsubai</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tsvetanov_Z/0/1/0/all/0/1">Zlatan I. Tsvetanov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pyrzas_S/0/1/0/all/0/1">Stylianos Pyrzas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Latham_D/0/1/0/all/0/1">David W. Latham</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bieryla_A/0/1/0/all/0/1">Allyson Bieryla</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Eastman_J/0/1/0/all/0/1">Jason Eastman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mislis_D/0/1/0/all/0/1">Dimitris Mislis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Esquerdo_G/0/1/0/all/0/1">Gilbert A. Esquerdo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Southworth_J/0/1/0/all/0/1">John Southworth</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mancini_L/0/1/0/all/0/1">Luigi Mancini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Esamdin_A/0/1/0/all/0/1">Ali Esamdin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Liu_J/0/1/0/all/0/1">Jinzhong […]

Cosmology and the Early Universe. (arXiv:1903.09260v1 [astro-ph.HE])

Cosmology and the Early Universe. (arXiv:1903.09260v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Sathyaprakash_B/0/1/0/all/0/1">B.S. Sathyaprakash</a> (Penn State and Cardiff University), <a href="http://arxiv.org/find/astro-ph/1/au:+Belgacem_E/0/1/0/all/0/1">Enis Belgacem</a> (University of Geneva), <a href="http://arxiv.org/find/astro-ph/1/au:+Bertacca_D/0/1/0/all/0/1">Daniele Bertacca</a> (Universita degli Studi di Padova), <a href="http://arxiv.org/find/astro-ph/1/au:+Caprini_C/0/1/0/all/0/1">Chiara Caprini</a> (Universite Paris Diderot, France), <a href="http://arxiv.org/find/astro-ph/1/au:+Cusin_G/0/1/0/all/0/1">Giulia Cusin</a> (University of Oxford, United Kingdom), <a href="http://arxiv.org/find/astro-ph/1/au:+Dirian_Y/0/1/0/all/0/1">Yves Dirian</a> (University of Geneva and University of Zuerich), <a […]

ZTF18aalrxas: A Type IIb Supernova from a very extended low-mass progenitor. (arXiv:1903.09262v1 [astro-ph.HE])

ZTF18aalrxas: A Type IIb Supernova from a very extended low-mass progenitor. (arXiv:1903.09262v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Fremling_C/0/1/0/all/0/1">C. Fremling</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ko_H/0/1/0/all/0/1">H. Ko</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dugas_A/0/1/0/all/0/1">A. Dugas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ergon_M/0/1/0/all/0/1">M. Ergon</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sollerman_J/0/1/0/all/0/1">J. Sollerman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bagdasaryan_A/0/1/0/all/0/1">A. Bagdasaryan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barbarino_C/0/1/0/all/0/1">C. Barbarino</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Belicki_J/0/1/0/all/0/1">J. Belicki</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bellm_E/0/1/0/all/0/1">E. Bellm</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Blagorodnova_N/0/1/0/all/0/1">N. Blagorodnova</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+De_K/0/1/0/all/0/1">K. De</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dekany_R/0/1/0/all/0/1">R. Dekany</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Frederick_S/0/1/0/all/0/1">S. Frederick</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gal_Yam_A/0/1/0/all/0/1">A. Gal-Yam</a>, […]

$nutexttt{bhlight}$: Radiation GRMHD for Neutrino-Driven Accretion Flows. (arXiv:1903.09273v1 [astro-ph.IM])

$nutexttt{bhlight}$: Radiation GRMHD for Neutrino-Driven Accretion Flows. (arXiv:1903.09273v1 [astro-ph.IM]) <a href="http://arxiv.org/find/astro-ph/1/au:+Miller_J/0/1/0/all/0/1">Jonah M. Miller</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ryan_B/0/1/0/all/0/1">Ben R. Ryan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dolence_J/0/1/0/all/0/1">Joshua C. Dolence</a> The 2017 detection of the in-spiral and merger of two neutron stars was a landmark discovery in astrophysics. We now know that such mergers are central engines of short gamma ray bursts and sites […]

Astro2020 Science White Paper: Local Dwarf Galaxy Archaeology. (arXiv:1903.09275v1 [astro-ph.GA])

Astro2020 Science White Paper: Local Dwarf Galaxy Archaeology. (arXiv:1903.09275v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Ji_A/0/1/0/all/0/1">Alexander P. Ji</a> (Carnegie Observatories), <a href="http://arxiv.org/find/astro-ph/1/au:+Beaton_R/0/1/0/all/0/1">Rachel Beaton</a> (Princeton University), <a href="http://arxiv.org/find/astro-ph/1/au:+Chakrabarti_S/0/1/0/all/0/1">Sukanya Chakrabarti</a> (RIT), <a href="http://arxiv.org/find/astro-ph/1/au:+Duggan_G/0/1/0/all/0/1">Gina Duggan</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Frebel_A/0/1/0/all/0/1">Anna Frebel</a> (MIT), <a href="http://arxiv.org/find/astro-ph/1/au:+Geha_M/0/1/0/all/0/1">Marla Geha</a> (Yale), <a href="http://arxiv.org/find/astro-ph/1/au:+Hosek_M/0/1/0/all/0/1">Matthew Hosek Jr</a> (UCLA), <a href="http://arxiv.org/find/astro-ph/1/au:+Kirby_E/0/1/0/all/0/1">Evan Kirby</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Li_T/0/1/0/all/0/1">Ting Li</a> (Fermilab), <a href="http://arxiv.org/find/astro-ph/1/au:+Roederer_I/0/1/0/all/0/1">Ian Roederer</a> (University of […]

Multimessenger Universe with Gravitational Waves from Binaries. (arXiv:1903.09277v1 [astro-ph.HE])

Multimessenger Universe with Gravitational Waves from Binaries. (arXiv:1903.09277v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Sathyaprakash_B/0/1/0/all/0/1">B.S. Sathyaprakash</a> (Penn State and Cardiff University), <a href="http://arxiv.org/find/astro-ph/1/au:+Bailes_M/0/1/0/all/0/1">Matthew Bailes</a> (Swinburne U.), <a href="http://arxiv.org/find/astro-ph/1/au:+Kasliwal_M/0/1/0/all/0/1">Mansi M. Kasliwal</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Nissanke_S/0/1/0/all/0/1">Samaya Nissanke</a> (U. of Amsterdam), <a href="http://arxiv.org/find/astro-ph/1/au:+Anand_S/0/1/0/all/0/1">Shreya Anand</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Andreoni_I/0/1/0/all/0/1">Igor Andreoni</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Colpi_M/0/1/0/all/0/1">Monica Colpi</a> (U. of Milano – Bicocca), <a href="http://arxiv.org/find/astro-ph/1/au:+Coughlin_M/0/1/0/all/0/1">Michael Coughlin</a> (Caltech), <a href="http://arxiv.org/find/astro-ph/1/au:+Hall_E/0/1/0/all/0/1">Evan […]

SDSS–IV MaNGA : The Inner Density Slopes of nearby galaxies. (arXiv:1903.09282v1 [astro-ph.GA])

SDSS–IV MaNGA : The Inner Density Slopes of nearby galaxies. (arXiv:1903.09282v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Li_R/0/1/0/all/0/1">Ran Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_H/0/1/0/all/0/1">Hongyu Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Shao_S/0/1/0/all/0/1">Shi Shao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lu_S/0/1/0/all/0/1">Shengdong Lu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhu_K/0/1/0/all/0/1">Kai Zhu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_C/0/1/0/all/0/1">Chunxiang Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gao_L/0/1/0/all/0/1">Liang Gao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mao_S/0/1/0/all/0/1">Shude Mao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dutton_A/0/1/0/all/0/1">Aaron A. Dutton</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ge_J/0/1/0/all/0/1">Junqiang Ge</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_Y/0/1/0/all/0/1">Yunchong Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Leauthaud_A/0/1/0/all/0/1">Alexie Leauthaud</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zheng_Z/0/1/0/all/0/1">Zheng Zheng</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bundy_K/0/1/0/all/0/1">Kevin Bundy</a>, […]

Detecting Offset Active Galactic Nuclei. (arXiv:1903.09301v1 [astro-ph.GA])

Detecting Offset Active Galactic Nuclei. (arXiv:1903.09301v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Blecha_L/0/1/0/all/0/1">Laura Blecha</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brisken_W/0/1/0/all/0/1">Walter Brisken</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Burke_Spolaor_S/0/1/0/all/0/1">Sarah Burke-Spolaor</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Civano_F/0/1/0/all/0/1">Francesca Civano</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Comerford_J/0/1/0/all/0/1">Julia Comerford</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Darling_J/0/1/0/all/0/1">Jeremy Darling</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lazio_T/0/1/0/all/0/1">T. Joseph W. Lazio</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Maccarone_T/0/1/0/all/0/1">Thomas J. Maccarone</a> Gravitational wave (GW) and gravitational slingshot recoil kicks, which are natural products of SMBH evolution in merging galaxies, can produce active […]

Understanding Accretion Outbursts in Massive Protostars through Maser Imaging. (arXiv:1903.09306v1 [astro-ph.SR])

Understanding Accretion Outbursts in Massive Protostars through Maser Imaging. (arXiv:1903.09306v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Hunter_T/0/1/0/all/0/1">Todd R. Hunter</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bartkiewicz_A/0/1/0/all/0/1">Anna Bartkiewicz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brisken_W/0/1/0/all/0/1">Walter Brisken</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brogan_C/0/1/0/all/0/1">Crystal L. Brogan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Burns_R/0/1/0/all/0/1">Ross Burns</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chibueze_J/0/1/0/all/0/1">James O. Chibueze</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cyganowski_C/0/1/0/all/0/1">Claudia J. Cyganowski</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hirota_T/0/1/0/all/0/1">Tomoya Hirota</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+MacLeod_G/0/1/0/all/0/1">Gordon MacLeod</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sanna_A/0/1/0/all/0/1">Alberto Sanna</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Torrelles_J/0/1/0/all/0/1">Jos&#xe9;-Mar&#xed;a Torrelles</a> The bright maser emission produced by several […]

Kinematics of the Galaxy from a Sample of Young Open Star Clusters with Data from the Gaia DR2 Catalogue. (arXiv:1903.09313v1 [astro-ph.GA])

Kinematics of the Galaxy from a Sample of Young Open Star Clusters with Data from the Gaia DR2 Catalogue. (arXiv:1903.09313v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Bobylev_V/0/1/0/all/0/1">V.V. Bobylev</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bajkova_A/0/1/0/all/0/1">A.T. Bajkova</a> We have selected a sample of 326 young $(log t

Ages and kinematics of chemically selected, accreted Milky Way halo stars. (arXiv:1903.09320v1 [astro-ph.GA])

Ages and kinematics of chemically selected, accreted Milky Way halo stars. (arXiv:1903.09320v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Das_P/0/1/0/all/0/1">Payel Das</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hawkins_K/0/1/0/all/0/1">Keith Hawkins</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jofre_P/0/1/0/all/0/1">Paula Jofre</a> We exploit the [Mg/Mn]-[Al/Fe] chemical abundance plane to help identify nearby halo stars in the 14th data release from the APOGEE survey that have been accreted on to the Milky Way. Applying a […]