Astrophysics is a science that employs the methods and principles of physics and chemistry in the study of astronomical objects and phenomena. As one of the founders of the discipline, James Keeler, said, astrophysics "seeks to ascertain the nature of the heavenly bodies, rather than their positions or motions in space–what they are, rather than where they are... Wikipedia

Conferences

Books

E-Books

The HDFC Library provides access to wide range of eBooks to support your research journey.
Use this E-Book guide to know how to access eBooks
The ProQuest eBooks central is major database having Neuroscience eBooks. List of some eBooks is given below:
(Note: To access books the below given books you must be logged in to eLibrary portal)

Journals

Referred Articles

ArticleDOI
Microstructure and the Pulsar Emission MechanismLink
Radio Observational Constraints on Pulsar Emission MechanismsLink
Radius-to-Frequency Mapping in the Radio Pulsar Emission MechanismLink
Crab Pulsar: Enhanced Optical Emission During Giant Radio PulsesLink
Radio spectra of millisecond pulsarsLink
Modelling the expected very high energy γ-ray emission from accreting neutron stars in X-ray binariesLink
Strange brewLink
Neutron Star Cooling and the Vela PulsarLink
The Current Status of Neutron Star Cooling TheoriesLink
Magnetic Field Effects upon Neutron Star CoolingLink
Gravitational Waves from Coalescing Neutron StarsLink
Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave eventLink
Wideband polarization and spectral properties of 18 high Galactic latitude pulsarsLink
Neutron Stars in the Light of Square Kilometre Array: Data, Statistics and ScienceLink
A lot of the periodic table is a result of neutron stars collidingLink
The dizziest, giddiest starsLink
Formation and Evolution of Ultraluminous X-Ray Pulsar Binaries to Pulsar–Neutron Star and Pulsar–White Dwarf SystemsLink
Pulsar Demography and Neutron Star AstrophysicsLink
Elastic and breaking properties of epitaxial face-centered crystals in neutron star crusts and white dwarf coresLink
Liquid-phase epitaxy of neutron star crusts and white dwarf coresLink
Study of Magnetic Field and Turbulence in the TeV Halo around the Monogem PulsarLink
Reciprocating Magnetic Fields in the Pulsar Wind Observed from the Black Widow Pulsar J1720-0534Link
A Spatially Resolved X-Ray Polarization Map of the Vela Pulsar Wind NebulaLink
Pulsar-based Galactic Magnetic Map: A Large-Scale Clockwise Magnetic Field with an Anticlockwise AnnulusLink
An XMM-Newton Observation of the High Magnetic Field Radio Pulsar PSR B0154+61Link
Chandra X-Ray Detection of the High Magnetic Field Radio Pulsar PSR J1718–3718Link
Pulsar radio emission mechanism: Why no consensus?Link
Toward an Empirical Theory of Pulsar Emission. XII. Exploring the Physical Conditions in Millisecond Pulsar Emission RegionsLink

Recent Trends

Internet/Blogs

TitleAccess
Deep learning prediction of galaxy stellar populations in the low-redshift UniverseLink
Chandra Peers Into Densest and Weirdest StarsLink
X-raying the Magnetic Field Bones of the Cosmic HandLink
A Magnetar-powered X-ray Transient as the Aftermath of a Binary Neutron-star MergerLink
A New Signal for a Neutron Star Collision DiscoveredLink
What are pulsars?Link
Pulsars and Their Glitches: A Glimpse into Neutron Star SecretsLink
This Extraordinary Celestial Structure Is The Product Of A Double SupernovaLink
A newly hatched neutron starLink
ASKAP searches for afterglow of gravitational waveLink
A chance encounter with a pulsarLink
Global collaboration is making waves in spaceLink
Fifty years ago Jocelyn Bell discovered pulsars and changed our view of the universeLink
Pulsar pays a flying visitLink
We counted 20 billion ticks of an extreme galactic clock to give Einstein’s theory of gravity its toughest test yetLink
Where are the missing gravitational waves?Link
Freaky pulsar flaunts its tailLink
neutron starsLink
THE COSMIC GIFT OF NEUTRON STARS: A LIVE-BLOG EVENTLink
The First Gravity Wave and Telescopic Neutron Star MergerLink

Visual sphere

Archive (Old Issues)

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